Pulsational pair instability as an explanation for the most luminous supernovae

Gespeichert in:

Autor*in:	Woosley, S.E. [verfasserIn] Blinnikov, S. Heger, Alexander

Format:	Artikel

Erschienen:	2007

Umfang:	3

Übergeordnetes Werk:	Enthalten in: Nature - London : Macmillan Publishers Limited, part of Springer Nature, 1869, 450(2007), 7168, Seite 390-392
Übergeordnetes Werk:	volume:450 ; year:2007 ; number:7168 ; pages:390-392 ; extent:3

Katalog-ID:	OLC1782319697

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allfieldsGer	sw071116 (DE-627)OLC1782319697 (DE-599)GBVOLC1782319697 DE-627 ger DE-627 rakwb 070 500 500 AVZ BIODIV fid Woosley, S.E. verfasserin aut Pulsational pair instability as an explanation for the most luminous supernovae 2007 3 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier Blinnikov, S. oth Heger, Alexander oth Enthalten in Nature London : Macmillan Publishers Limited, part of Springer Nature, 1869 450(2007), 7168, Seite 390-392 (DE-627)129292834 (DE-600)120714-3 (DE-576)014473941 0028-0836 nnns volume:450 year:2007 number:7168 pages:390-392 extent:3 GBV_USEFLAG_A SYSFLAG_A GBV_OLC FID-BIODIV SSG-OLC-PHY SSG-OLC-CHE SSG-OLC-MAT SSG-OLC-FOR SSG-OLC-SPO SSG-OLC-PHA SSG-OLC-DE-84 SSG-OPC-FOR GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_23 GBV_ILN_30 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_47 GBV_ILN_55 GBV_ILN_59 GBV_ILN_60 GBV_ILN_62 GBV_ILN_69 GBV_ILN_70 GBV_ILN_95 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_130 GBV_ILN_150 GBV_ILN_154 GBV_ILN_168 GBV_ILN_170 GBV_ILN_171 GBV_ILN_211 GBV_ILN_215 GBV_ILN_285 GBV_ILN_290 GBV_ILN_601 GBV_ILN_647 GBV_ILN_702 GBV_ILN_754 GBV_ILN_2002 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2008 GBV_ILN_2010 GBV_ILN_2012 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2016 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2027 GBV_ILN_2095 GBV_ILN_2120 GBV_ILN_2121 GBV_ILN_2173 GBV_ILN_2219 GBV_ILN_2221 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_2360 GBV_ILN_2410 GBV_ILN_2411 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4219 GBV_ILN_4277 GBV_ILN_4302 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4311 GBV_ILN_4314 GBV_ILN_4315 GBV_ILN_4317 GBV_ILN_4318 GBV_ILN_4320 GBV_ILN_4323 GBV_ILN_4385 GBV_ILN_4598 GBV_ILN_4700 AR 450 2007 7168 390-392 3
allfieldsSound	sw071116 (DE-627)OLC1782319697 (DE-599)GBVOLC1782319697 DE-627 ger DE-627 rakwb 070 500 500 AVZ BIODIV fid Woosley, S.E. verfasserin aut Pulsational pair instability as an explanation for the most luminous supernovae 2007 3 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier Blinnikov, S. oth Heger, Alexander oth Enthalten in Nature London : Macmillan Publishers Limited, part of Springer Nature, 1869 450(2007), 7168, Seite 390-392 (DE-627)129292834 (DE-600)120714-3 (DE-576)014473941 0028-0836 nnns volume:450 year:2007 number:7168 pages:390-392 extent:3 GBV_USEFLAG_A SYSFLAG_A GBV_OLC FID-BIODIV SSG-OLC-PHY SSG-OLC-CHE SSG-OLC-MAT SSG-OLC-FOR SSG-OLC-SPO SSG-OLC-PHA SSG-OLC-DE-84 SSG-OPC-FOR GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_23 GBV_ILN_30 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_47 GBV_ILN_55 GBV_ILN_59 GBV_ILN_60 GBV_ILN_62 GBV_ILN_69 GBV_ILN_70 GBV_ILN_95 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_130 GBV_ILN_150 GBV_ILN_154 GBV_ILN_168 GBV_ILN_170 GBV_ILN_171 GBV_ILN_211 GBV_ILN_215 GBV_ILN_285 GBV_ILN_290 GBV_ILN_601 GBV_ILN_647 GBV_ILN_702 GBV_ILN_754 GBV_ILN_2002 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2008 GBV_ILN_2010 GBV_ILN_2012 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2016 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2027 GBV_ILN_2095 GBV_ILN_2120 GBV_ILN_2121 GBV_ILN_2173 GBV_ILN_2219 GBV_ILN_2221 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_2360 GBV_ILN_2410 GBV_ILN_2411 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4219 GBV_ILN_4277 GBV_ILN_4302 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4311 GBV_ILN_4314 GBV_ILN_4315 GBV_ILN_4317 GBV_ILN_4318 GBV_ILN_4320 GBV_ILN_4323 GBV_ILN_4385 GBV_ILN_4598 GBV_ILN_4700 AR 450 2007 7168 390-392 3
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title	Pulsational pair instability as an explanation for the most luminous supernovae
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title_short	Pulsational pair instability as an explanation for the most luminous supernovae
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Pulsational pair instability as an explanation for the most luminous supernovae

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