Underground Measurements of Nuclear Reaction Cross-Sections Relevant to AGB Stars

Nuclear reaction cross sections are essential ingredients to predict the evolution of AGB stars and understand their impact on the chemical evolution of our Galaxy. Unfortunately, the cross sections of the reactions involved are often very small and challenging to measure in laboratories on Earth. I...
Ausführliche Beschreibung

Gespeichert in:

Autor*in:	Chemseddine Ananna [verfasserIn] Francesco Barile [verfasserIn] Axel Boeltzig [verfasserIn] Carlo Giulio Bruno [verfasserIn] Francesca Cavanna [verfasserIn] Giovanni Francesco Ciani [verfasserIn] Alessandro Compagnucci [verfasserIn] Laszlo Csedreki [verfasserIn] Rosanna Depalo [verfasserIn] Federico Ferraro [verfasserIn] Eliana Masha [verfasserIn] Denise Piatti [verfasserIn] David Rapagnani [verfasserIn] Jakub Skowronski [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2021

Schlagwörter:	Underground Nuclear Astrophysics stellar evolution stellar nucleosynthesis

Übergeordnetes Werk:	In: Universe - MDPI AG, 2015, 8(2021), 1, p 4
Übergeordnetes Werk:	volume:8 ; year:2021 ; number:1, p 4

Links:	Link aufrufen Link aufrufen Link aufrufen Journal toc

DOI / URN:	10.3390/universe8010004

Katalog-ID:	DOAJ023456795

Internformat


LEADER	01000caa a22002652 4500
001	DOAJ023456795
003	DE-627
005	20240414205629.0
007	cr uuu---uuuuu
008	230226s2021 xx \|\|\|\|\|o 00\| \|\|eng c
024	7		\|a 10.3390/universe8010004 \|2 doi
035			\|a (DE-627)DOAJ023456795
035			\|a (DE-599)DOAJ89e00d25f42e4ab5b42b0adf31d3d80e
040			\|a DE-627 \|b ger \|c DE-627 \|e rakwb
041			\|a eng
050		0	\|a QC793-793.5
100	0		\|a Chemseddine Ananna \|e verfasserin \|4 aut
245	1	0	\|a Underground Measurements of Nuclear Reaction Cross-Sections Relevant to AGB Stars
264		1	\|c 2021
336			\|a Text \|b txt \|2 rdacontent
337			\|a Computermedien \|b c \|2 rdamedia
338			\|a Online-Ressource \|b cr \|2 rdacarrier
520			\|a Nuclear reaction cross sections are essential ingredients to predict the evolution of AGB stars and understand their impact on the chemical evolution of our Galaxy. Unfortunately, the cross sections of the reactions involved are often very small and challenging to measure in laboratories on Earth. In this context, major steps forward were made with the advent of underground nuclear astrophysics, pioneered by the Laboratory for Underground Nuclear Astrophysics (LUNA). The present paper reviews the contribution of LUNA to our understanding of the evolution of AGB stars and related nucleosynthesis.
650		4	\|a Underground Nuclear Astrophysics
650		4	\|a stellar evolution
650		4	\|a stellar nucleosynthesis
653		0	\|a Elementary particle physics
700	0		\|a Francesco Barile \|e verfasserin \|4 aut
700	0		\|a Axel Boeltzig \|e verfasserin \|4 aut
700	0		\|a Carlo Giulio Bruno \|e verfasserin \|4 aut
700	0		\|a Francesca Cavanna \|e verfasserin \|4 aut
700	0		\|a Giovanni Francesco Ciani \|e verfasserin \|4 aut
700	0		\|a Alessandro Compagnucci \|e verfasserin \|4 aut
700	0		\|a Laszlo Csedreki \|e verfasserin \|4 aut
700	0		\|a Rosanna Depalo \|e verfasserin \|4 aut
700	0		\|a Federico Ferraro \|e verfasserin \|4 aut
700	0		\|a Eliana Masha \|e verfasserin \|4 aut
700	0		\|a Denise Piatti \|e verfasserin \|4 aut
700	0		\|a David Rapagnani \|e verfasserin \|4 aut
700	0		\|a Jakub Skowronski \|e verfasserin \|4 aut
773	0	8	\|i In \|t Universe \|d MDPI AG, 2015 \|g 8(2021), 1, p 4 \|w (DE-627)820684236 \|w (DE-600)2813994-X \|x 22181997 \|7 nnns
773	1	8	\|g volume:8 \|g year:2021 \|g number:1, p 4
856	4	0	\|u https://doi.org/10.3390/universe8010004 \|z kostenfrei
856	4	0	\|u https://doaj.org/article/89e00d25f42e4ab5b42b0adf31d3d80e \|z kostenfrei
856	4	0	\|u https://www.mdpi.com/2218-1997/8/1/4 \|z kostenfrei
856	4	2	\|u https://doaj.org/toc/2218-1997 \|y Journal toc \|z kostenfrei
912			\|a GBV_USEFLAG_A
912			\|a SYSFLAG_A
912			\|a GBV_DOAJ
912			\|a GBV_ILN_20
912			\|a GBV_ILN_22
912			\|a GBV_ILN_23
912			\|a GBV_ILN_24
912			\|a GBV_ILN_39
912			\|a GBV_ILN_40
912			\|a GBV_ILN_60
912			\|a GBV_ILN_62
912			\|a GBV_ILN_63
912			\|a GBV_ILN_65
912			\|a GBV_ILN_69
912			\|a GBV_ILN_70
912			\|a GBV_ILN_73
912			\|a GBV_ILN_95
912			\|a GBV_ILN_105
912			\|a GBV_ILN_110
912			\|a GBV_ILN_151
912			\|a GBV_ILN_161
912			\|a GBV_ILN_170
912			\|a GBV_ILN_213
912			\|a GBV_ILN_230
912			\|a GBV_ILN_285
912			\|a GBV_ILN_293
912			\|a GBV_ILN_370
912			\|a GBV_ILN_602
912			\|a GBV_ILN_2005
912			\|a GBV_ILN_2009
912			\|a GBV_ILN_2014
912			\|a GBV_ILN_2055
912			\|a GBV_ILN_2111
912			\|a GBV_ILN_4012
912			\|a GBV_ILN_4037
912			\|a GBV_ILN_4112
912			\|a GBV_ILN_4125
912			\|a GBV_ILN_4126
912			\|a GBV_ILN_4249
912			\|a GBV_ILN_4305
912			\|a GBV_ILN_4306
912			\|a GBV_ILN_4307
912			\|a GBV_ILN_4313
912			\|a GBV_ILN_4322
912			\|a GBV_ILN_4323
912			\|a GBV_ILN_4324
912			\|a GBV_ILN_4325
912			\|a GBV_ILN_4335
912			\|a GBV_ILN_4338
912			\|a GBV_ILN_4367
912			\|a GBV_ILN_4700
951			\|a AR
952			\|d 8 \|j 2021 \|e 1, p 4

Indexfelder

author_variant	c a ca f b fb a b ab c g b cgb f c fc g f c gfc a c ac l c lc r d rd f f ff e m em d p dp d r dr j s js
matchkey_str	article:22181997:2021----::negonmaueetoncerecinrssci
hierarchy_sort_str	2021
callnumber-subject-code	QC
publishDate	2021
allfields	10.3390/universe8010004 doi (DE-627)DOAJ023456795 (DE-599)DOAJ89e00d25f42e4ab5b42b0adf31d3d80e DE-627 ger DE-627 rakwb eng QC793-793.5 Chemseddine Ananna verfasserin aut Underground Measurements of Nuclear Reaction Cross-Sections Relevant to AGB Stars 2021 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Nuclear reaction cross sections are essential ingredients to predict the evolution of AGB stars and understand their impact on the chemical evolution of our Galaxy. Unfortunately, the cross sections of the reactions involved are often very small and challenging to measure in laboratories on Earth. In this context, major steps forward were made with the advent of underground nuclear astrophysics, pioneered by the Laboratory for Underground Nuclear Astrophysics (LUNA). The present paper reviews the contribution of LUNA to our understanding of the evolution of AGB stars and related nucleosynthesis. Underground Nuclear Astrophysics stellar evolution stellar nucleosynthesis Elementary particle physics Francesco Barile verfasserin aut Axel Boeltzig verfasserin aut Carlo Giulio Bruno verfasserin aut Francesca Cavanna verfasserin aut Giovanni Francesco Ciani verfasserin aut Alessandro Compagnucci verfasserin aut Laszlo Csedreki verfasserin aut Rosanna Depalo verfasserin aut Federico Ferraro verfasserin aut Eliana Masha verfasserin aut Denise Piatti verfasserin aut David Rapagnani verfasserin aut Jakub Skowronski verfasserin aut In Universe MDPI AG, 2015 8(2021), 1, p 4 (DE-627)820684236 (DE-600)2813994-X 22181997 nnns volume:8 year:2021 number:1, p 4 https://doi.org/10.3390/universe8010004 kostenfrei https://doaj.org/article/89e00d25f42e4ab5b42b0adf31d3d80e kostenfrei https://www.mdpi.com/2218-1997/8/1/4 kostenfrei https://doaj.org/toc/2218-1997 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2005 GBV_ILN_2009 GBV_ILN_2014 GBV_ILN_2055 GBV_ILN_2111 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 8 2021 1, p 4
spelling	10.3390/universe8010004 doi (DE-627)DOAJ023456795 (DE-599)DOAJ89e00d25f42e4ab5b42b0adf31d3d80e DE-627 ger DE-627 rakwb eng QC793-793.5 Chemseddine Ananna verfasserin aut Underground Measurements of Nuclear Reaction Cross-Sections Relevant to AGB Stars 2021 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Nuclear reaction cross sections are essential ingredients to predict the evolution of AGB stars and understand their impact on the chemical evolution of our Galaxy. Unfortunately, the cross sections of the reactions involved are often very small and challenging to measure in laboratories on Earth. In this context, major steps forward were made with the advent of underground nuclear astrophysics, pioneered by the Laboratory for Underground Nuclear Astrophysics (LUNA). The present paper reviews the contribution of LUNA to our understanding of the evolution of AGB stars and related nucleosynthesis. Underground Nuclear Astrophysics stellar evolution stellar nucleosynthesis Elementary particle physics Francesco Barile verfasserin aut Axel Boeltzig verfasserin aut Carlo Giulio Bruno verfasserin aut Francesca Cavanna verfasserin aut Giovanni Francesco Ciani verfasserin aut Alessandro Compagnucci verfasserin aut Laszlo Csedreki verfasserin aut Rosanna Depalo verfasserin aut Federico Ferraro verfasserin aut Eliana Masha verfasserin aut Denise Piatti verfasserin aut David Rapagnani verfasserin aut Jakub Skowronski verfasserin aut In Universe MDPI AG, 2015 8(2021), 1, p 4 (DE-627)820684236 (DE-600)2813994-X 22181997 nnns volume:8 year:2021 number:1, p 4 https://doi.org/10.3390/universe8010004 kostenfrei https://doaj.org/article/89e00d25f42e4ab5b42b0adf31d3d80e kostenfrei https://www.mdpi.com/2218-1997/8/1/4 kostenfrei https://doaj.org/toc/2218-1997 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2005 GBV_ILN_2009 GBV_ILN_2014 GBV_ILN_2055 GBV_ILN_2111 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 8 2021 1, p 4
allfields_unstemmed	10.3390/universe8010004 doi (DE-627)DOAJ023456795 (DE-599)DOAJ89e00d25f42e4ab5b42b0adf31d3d80e DE-627 ger DE-627 rakwb eng QC793-793.5 Chemseddine Ananna verfasserin aut Underground Measurements of Nuclear Reaction Cross-Sections Relevant to AGB Stars 2021 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Nuclear reaction cross sections are essential ingredients to predict the evolution of AGB stars and understand their impact on the chemical evolution of our Galaxy. Unfortunately, the cross sections of the reactions involved are often very small and challenging to measure in laboratories on Earth. In this context, major steps forward were made with the advent of underground nuclear astrophysics, pioneered by the Laboratory for Underground Nuclear Astrophysics (LUNA). The present paper reviews the contribution of LUNA to our understanding of the evolution of AGB stars and related nucleosynthesis. Underground Nuclear Astrophysics stellar evolution stellar nucleosynthesis Elementary particle physics Francesco Barile verfasserin aut Axel Boeltzig verfasserin aut Carlo Giulio Bruno verfasserin aut Francesca Cavanna verfasserin aut Giovanni Francesco Ciani verfasserin aut Alessandro Compagnucci verfasserin aut Laszlo Csedreki verfasserin aut Rosanna Depalo verfasserin aut Federico Ferraro verfasserin aut Eliana Masha verfasserin aut Denise Piatti verfasserin aut David Rapagnani verfasserin aut Jakub Skowronski verfasserin aut In Universe MDPI AG, 2015 8(2021), 1, p 4 (DE-627)820684236 (DE-600)2813994-X 22181997 nnns volume:8 year:2021 number:1, p 4 https://doi.org/10.3390/universe8010004 kostenfrei https://doaj.org/article/89e00d25f42e4ab5b42b0adf31d3d80e kostenfrei https://www.mdpi.com/2218-1997/8/1/4 kostenfrei https://doaj.org/toc/2218-1997 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2005 GBV_ILN_2009 GBV_ILN_2014 GBV_ILN_2055 GBV_ILN_2111 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 8 2021 1, p 4
allfieldsGer	10.3390/universe8010004 doi (DE-627)DOAJ023456795 (DE-599)DOAJ89e00d25f42e4ab5b42b0adf31d3d80e DE-627 ger DE-627 rakwb eng QC793-793.5 Chemseddine Ananna verfasserin aut Underground Measurements of Nuclear Reaction Cross-Sections Relevant to AGB Stars 2021 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Nuclear reaction cross sections are essential ingredients to predict the evolution of AGB stars and understand their impact on the chemical evolution of our Galaxy. Unfortunately, the cross sections of the reactions involved are often very small and challenging to measure in laboratories on Earth. In this context, major steps forward were made with the advent of underground nuclear astrophysics, pioneered by the Laboratory for Underground Nuclear Astrophysics (LUNA). The present paper reviews the contribution of LUNA to our understanding of the evolution of AGB stars and related nucleosynthesis. Underground Nuclear Astrophysics stellar evolution stellar nucleosynthesis Elementary particle physics Francesco Barile verfasserin aut Axel Boeltzig verfasserin aut Carlo Giulio Bruno verfasserin aut Francesca Cavanna verfasserin aut Giovanni Francesco Ciani verfasserin aut Alessandro Compagnucci verfasserin aut Laszlo Csedreki verfasserin aut Rosanna Depalo verfasserin aut Federico Ferraro verfasserin aut Eliana Masha verfasserin aut Denise Piatti verfasserin aut David Rapagnani verfasserin aut Jakub Skowronski verfasserin aut In Universe MDPI AG, 2015 8(2021), 1, p 4 (DE-627)820684236 (DE-600)2813994-X 22181997 nnns volume:8 year:2021 number:1, p 4 https://doi.org/10.3390/universe8010004 kostenfrei https://doaj.org/article/89e00d25f42e4ab5b42b0adf31d3d80e kostenfrei https://www.mdpi.com/2218-1997/8/1/4 kostenfrei https://doaj.org/toc/2218-1997 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2005 GBV_ILN_2009 GBV_ILN_2014 GBV_ILN_2055 GBV_ILN_2111 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 8 2021 1, p 4
allfieldsSound	10.3390/universe8010004 doi (DE-627)DOAJ023456795 (DE-599)DOAJ89e00d25f42e4ab5b42b0adf31d3d80e DE-627 ger DE-627 rakwb eng QC793-793.5 Chemseddine Ananna verfasserin aut Underground Measurements of Nuclear Reaction Cross-Sections Relevant to AGB Stars 2021 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Nuclear reaction cross sections are essential ingredients to predict the evolution of AGB stars and understand their impact on the chemical evolution of our Galaxy. Unfortunately, the cross sections of the reactions involved are often very small and challenging to measure in laboratories on Earth. In this context, major steps forward were made with the advent of underground nuclear astrophysics, pioneered by the Laboratory for Underground Nuclear Astrophysics (LUNA). The present paper reviews the contribution of LUNA to our understanding of the evolution of AGB stars and related nucleosynthesis. Underground Nuclear Astrophysics stellar evolution stellar nucleosynthesis Elementary particle physics Francesco Barile verfasserin aut Axel Boeltzig verfasserin aut Carlo Giulio Bruno verfasserin aut Francesca Cavanna verfasserin aut Giovanni Francesco Ciani verfasserin aut Alessandro Compagnucci verfasserin aut Laszlo Csedreki verfasserin aut Rosanna Depalo verfasserin aut Federico Ferraro verfasserin aut Eliana Masha verfasserin aut Denise Piatti verfasserin aut David Rapagnani verfasserin aut Jakub Skowronski verfasserin aut In Universe MDPI AG, 2015 8(2021), 1, p 4 (DE-627)820684236 (DE-600)2813994-X 22181997 nnns volume:8 year:2021 number:1, p 4 https://doi.org/10.3390/universe8010004 kostenfrei https://doaj.org/article/89e00d25f42e4ab5b42b0adf31d3d80e kostenfrei https://www.mdpi.com/2218-1997/8/1/4 kostenfrei https://doaj.org/toc/2218-1997 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2005 GBV_ILN_2009 GBV_ILN_2014 GBV_ILN_2055 GBV_ILN_2111 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 8 2021 1, p 4
language	English
source	In Universe 8(2021), 1, p 4 volume:8 year:2021 number:1, p 4
sourceStr	In Universe 8(2021), 1, p 4 volume:8 year:2021 number:1, p 4
format_phy_str_mv	Article
institution	findex.gbv.de
topic_facet	Underground Nuclear Astrophysics stellar evolution stellar nucleosynthesis Elementary particle physics
isfreeaccess_bool	true
container_title	Universe
authorswithroles_txt_mv	Chemseddine Ananna @@aut@@ Francesco Barile @@aut@@ Axel Boeltzig @@aut@@ Carlo Giulio Bruno @@aut@@ Francesca Cavanna @@aut@@ Giovanni Francesco Ciani @@aut@@ Alessandro Compagnucci @@aut@@ Laszlo Csedreki @@aut@@ Rosanna Depalo @@aut@@ Federico Ferraro @@aut@@ Eliana Masha @@aut@@ Denise Piatti @@aut@@ David Rapagnani @@aut@@ Jakub Skowronski @@aut@@
publishDateDaySort_date	2021-01-01T00:00:00Z
hierarchy_top_id	820684236
id	DOAJ023456795
language_de	englisch
fullrecord	<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">DOAJ023456795</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20240414205629.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">230226s2021 xx \|\|\|\|\|o 00\| \|\|eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.3390/universe8010004</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)DOAJ023456795</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)DOAJ89e00d25f42e4ab5b42b0adf31d3d80e</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="050" ind1=" " ind2="0"><subfield code="a">QC793-793.5</subfield></datafield><datafield tag="100" ind1="0" ind2=" "><subfield code="a">Chemseddine Ananna</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Underground Measurements of Nuclear Reaction Cross-Sections Relevant to AGB Stars</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2021</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">Computermedien</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Nuclear reaction cross sections are essential ingredients to predict the evolution of AGB stars and understand their impact on the chemical evolution of our Galaxy. Unfortunately, the cross sections of the reactions involved are often very small and challenging to measure in laboratories on Earth. In this context, major steps forward were made with the advent of underground nuclear astrophysics, pioneered by the Laboratory for Underground Nuclear Astrophysics (LUNA). The present paper reviews the contribution of LUNA to our understanding of the evolution of AGB stars and related nucleosynthesis.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Underground Nuclear Astrophysics</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">stellar evolution</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">stellar nucleosynthesis</subfield></datafield><datafield tag="653" ind1=" " ind2="0"><subfield code="a">Elementary particle physics</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">Francesco Barile</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">Axel Boeltzig</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">Carlo Giulio Bruno</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">Francesca Cavanna</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">Giovanni Francesco Ciani</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">Alessandro Compagnucci</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">Laszlo Csedreki</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">Rosanna Depalo</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">Federico Ferraro</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">Eliana Masha</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">Denise Piatti</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">David Rapagnani</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">Jakub Skowronski</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">In</subfield><subfield code="t">Universe</subfield><subfield code="d">MDPI AG, 2015</subfield><subfield code="g">8(2021), 1, p 4</subfield><subfield code="w">(DE-627)820684236</subfield><subfield code="w">(DE-600)2813994-X</subfield><subfield code="x">22181997</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:8</subfield><subfield code="g">year:2021</subfield><subfield code="g">number:1, p 4</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://doi.org/10.3390/universe8010004</subfield><subfield code="z">kostenfrei</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://doaj.org/article/89e00d25f42e4ab5b42b0adf31d3d80e</subfield><subfield code="z">kostenfrei</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://www.mdpi.com/2218-1997/8/1/4</subfield><subfield code="z">kostenfrei</subfield></datafield><datafield tag="856" ind1="4" ind2="2"><subfield code="u">https://doaj.org/toc/2218-1997</subfield><subfield code="y">Journal toc</subfield><subfield code="z">kostenfrei</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SYSFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_DOAJ</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_20</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_22</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_23</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_24</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_39</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_40</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_60</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_62</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_63</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_65</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_69</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_70</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_73</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_95</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_105</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_110</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_151</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_161</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_170</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_213</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_230</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_285</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_293</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_370</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_602</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2005</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2009</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2014</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2055</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2111</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4012</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4037</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4112</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4125</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4126</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4249</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4305</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4306</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4307</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4313</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4322</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4323</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4324</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4325</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4335</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4338</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4367</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4700</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">8</subfield><subfield code="j">2021</subfield><subfield code="e">1, p 4</subfield></datafield></record></collection>
callnumber-first	Q - Science
author	Chemseddine Ananna
spellingShingle	Chemseddine Ananna misc QC793-793.5 misc Underground Nuclear Astrophysics misc stellar evolution misc stellar nucleosynthesis misc Elementary particle physics Underground Measurements of Nuclear Reaction Cross-Sections Relevant to AGB Stars
authorStr	Chemseddine Ananna
ppnlink_with_tag_str_mv	@@773@@(DE-627)820684236
format	electronic Article
delete_txt_mv	keep
author_role	aut aut aut aut aut aut aut aut aut aut aut aut aut aut
collection	DOAJ
remote_str	true
callnumber-label	QC793-793
illustrated	Not Illustrated
issn	22181997
topic_title	QC793-793.5 Underground Measurements of Nuclear Reaction Cross-Sections Relevant to AGB Stars Underground Nuclear Astrophysics stellar evolution stellar nucleosynthesis
topic	misc QC793-793.5 misc Underground Nuclear Astrophysics misc stellar evolution misc stellar nucleosynthesis misc Elementary particle physics
topic_unstemmed	misc QC793-793.5 misc Underground Nuclear Astrophysics misc stellar evolution misc stellar nucleosynthesis misc Elementary particle physics
topic_browse	misc QC793-793.5 misc Underground Nuclear Astrophysics misc stellar evolution misc stellar nucleosynthesis misc Elementary particle physics
format_facet	Elektronische Aufsätze Aufsätze Elektronische Ressource
format_main_str_mv	Text Zeitschrift/Artikel
carriertype_str_mv	cr
hierarchy_parent_title	Universe
hierarchy_parent_id	820684236
hierarchy_top_title	Universe
isfreeaccess_txt	true
familylinks_str_mv	(DE-627)820684236 (DE-600)2813994-X
title	Underground Measurements of Nuclear Reaction Cross-Sections Relevant to AGB Stars
ctrlnum	(DE-627)DOAJ023456795 (DE-599)DOAJ89e00d25f42e4ab5b42b0adf31d3d80e
title_full	Underground Measurements of Nuclear Reaction Cross-Sections Relevant to AGB Stars
author_sort	Chemseddine Ananna
journal	Universe
journalStr	Universe
callnumber-first-code	Q
lang_code	eng
isOA_bool	true
recordtype	marc
publishDateSort	2021
contenttype_str_mv	txt
author_browse	Chemseddine Ananna Francesco Barile Axel Boeltzig Carlo Giulio Bruno Francesca Cavanna Giovanni Francesco Ciani Alessandro Compagnucci Laszlo Csedreki Rosanna Depalo Federico Ferraro Eliana Masha Denise Piatti David Rapagnani Jakub Skowronski
container_volume	8
class	QC793-793.5
format_se	Elektronische Aufsätze
author-letter	Chemseddine Ananna
doi_str_mv	10.3390/universe8010004
author2-role	verfasserin
title_sort	underground measurements of nuclear reaction cross-sections relevant to agb stars
callnumber	QC793-793.5
title_auth	Underground Measurements of Nuclear Reaction Cross-Sections Relevant to AGB Stars
abstract	Nuclear reaction cross sections are essential ingredients to predict the evolution of AGB stars and understand their impact on the chemical evolution of our Galaxy. Unfortunately, the cross sections of the reactions involved are often very small and challenging to measure in laboratories on Earth. In this context, major steps forward were made with the advent of underground nuclear astrophysics, pioneered by the Laboratory for Underground Nuclear Astrophysics (LUNA). The present paper reviews the contribution of LUNA to our understanding of the evolution of AGB stars and related nucleosynthesis.
abstractGer	Nuclear reaction cross sections are essential ingredients to predict the evolution of AGB stars and understand their impact on the chemical evolution of our Galaxy. Unfortunately, the cross sections of the reactions involved are often very small and challenging to measure in laboratories on Earth. In this context, major steps forward were made with the advent of underground nuclear astrophysics, pioneered by the Laboratory for Underground Nuclear Astrophysics (LUNA). The present paper reviews the contribution of LUNA to our understanding of the evolution of AGB stars and related nucleosynthesis.
abstract_unstemmed	Nuclear reaction cross sections are essential ingredients to predict the evolution of AGB stars and understand their impact on the chemical evolution of our Galaxy. Unfortunately, the cross sections of the reactions involved are often very small and challenging to measure in laboratories on Earth. In this context, major steps forward were made with the advent of underground nuclear astrophysics, pioneered by the Laboratory for Underground Nuclear Astrophysics (LUNA). The present paper reviews the contribution of LUNA to our understanding of the evolution of AGB stars and related nucleosynthesis.
collection_details	GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2005 GBV_ILN_2009 GBV_ILN_2014 GBV_ILN_2055 GBV_ILN_2111 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700
container_issue	1, p 4
title_short	Underground Measurements of Nuclear Reaction Cross-Sections Relevant to AGB Stars
url	https://doi.org/10.3390/universe8010004 https://doaj.org/article/89e00d25f42e4ab5b42b0adf31d3d80e https://www.mdpi.com/2218-1997/8/1/4 https://doaj.org/toc/2218-1997
remote_bool	true
author2	Francesco Barile Axel Boeltzig Carlo Giulio Bruno Francesca Cavanna Giovanni Francesco Ciani Alessandro Compagnucci Laszlo Csedreki Rosanna Depalo Federico Ferraro Eliana Masha Denise Piatti David Rapagnani Jakub Skowronski
author2Str	Francesco Barile Axel Boeltzig Carlo Giulio Bruno Francesca Cavanna Giovanni Francesco Ciani Alessandro Compagnucci Laszlo Csedreki Rosanna Depalo Federico Ferraro Eliana Masha Denise Piatti David Rapagnani Jakub Skowronski
ppnlink	820684236
callnumber-subject	QC - Physics
mediatype_str_mv	c
isOA_txt	true
hochschulschrift_bool	false
doi_str	10.3390/universe8010004
callnumber-a	QC793-793.5
up_date	2024-07-03T17:42:38.135Z
_version_	1803580665374965760
fullrecord_marcxml	<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">DOAJ023456795</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20240414205629.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">230226s2021 xx \|\|\|\|\|o 00\| \|\|eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.3390/universe8010004</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)DOAJ023456795</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)DOAJ89e00d25f42e4ab5b42b0adf31d3d80e</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="050" ind1=" " ind2="0"><subfield code="a">QC793-793.5</subfield></datafield><datafield tag="100" ind1="0" ind2=" "><subfield code="a">Chemseddine Ananna</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Underground Measurements of Nuclear Reaction Cross-Sections Relevant to AGB Stars</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2021</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">Computermedien</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Nuclear reaction cross sections are essential ingredients to predict the evolution of AGB stars and understand their impact on the chemical evolution of our Galaxy. Unfortunately, the cross sections of the reactions involved are often very small and challenging to measure in laboratories on Earth. In this context, major steps forward were made with the advent of underground nuclear astrophysics, pioneered by the Laboratory for Underground Nuclear Astrophysics (LUNA). The present paper reviews the contribution of LUNA to our understanding of the evolution of AGB stars and related nucleosynthesis.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Underground Nuclear Astrophysics</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">stellar evolution</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">stellar nucleosynthesis</subfield></datafield><datafield tag="653" ind1=" " ind2="0"><subfield code="a">Elementary particle physics</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">Francesco Barile</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">Axel Boeltzig</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">Carlo Giulio Bruno</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">Francesca Cavanna</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">Giovanni Francesco Ciani</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">Alessandro Compagnucci</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">Laszlo Csedreki</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">Rosanna Depalo</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">Federico Ferraro</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">Eliana Masha</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">Denise Piatti</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">David Rapagnani</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">Jakub Skowronski</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">In</subfield><subfield code="t">Universe</subfield><subfield code="d">MDPI AG, 2015</subfield><subfield code="g">8(2021), 1, p 4</subfield><subfield code="w">(DE-627)820684236</subfield><subfield code="w">(DE-600)2813994-X</subfield><subfield code="x">22181997</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:8</subfield><subfield code="g">year:2021</subfield><subfield code="g">number:1, p 4</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://doi.org/10.3390/universe8010004</subfield><subfield code="z">kostenfrei</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://doaj.org/article/89e00d25f42e4ab5b42b0adf31d3d80e</subfield><subfield code="z">kostenfrei</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://www.mdpi.com/2218-1997/8/1/4</subfield><subfield code="z">kostenfrei</subfield></datafield><datafield tag="856" ind1="4" ind2="2"><subfield code="u">https://doaj.org/toc/2218-1997</subfield><subfield code="y">Journal toc</subfield><subfield code="z">kostenfrei</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SYSFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_DOAJ</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_20</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_22</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_23</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_24</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_39</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_40</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_60</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_62</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_63</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_65</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_69</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_70</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_73</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_95</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_105</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_110</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_151</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_161</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_170</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_213</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_230</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_285</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_293</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_370</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_602</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2005</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2009</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2014</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2055</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2111</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4012</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4037</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4112</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4125</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4126</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4249</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4305</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4306</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4307</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4313</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4322</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4323</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4324</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4325</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4335</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4338</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4367</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4700</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">8</subfield><subfield code="j">2021</subfield><subfield code="e">1, p 4</subfield></datafield></record></collection>
score	7.4028025

Nicht das Richtige dabei?

Schreiben Sie uns!

Underground Measurements of Nuclear Reaction Cross-Sections Relevant to AGB Stars

Nicht das Richtige dabei?

Zugang & Verfügbarkeit

Vorhandene Bände

Nicht das Richtige dabei?