Constraining Star-Formation Driven Outflows in Local Dwarf Galaxies with <i<Herschel</i<<xref rid="fn1-psf-2287691" ref-type="fn"<†</xref<
Galactic feedback (i.e., outflows) plays a fundamental role in regulating galaxy formation and evolution. We investigate the physical properties of galactic outflows in a sample of 29 local low-metallicity dwarf galaxies drawn from the Dwarf Galaxy Survey. We make use of Herschel/PACS archival data...
Ausführliche Beschreibung
Autor*in: |
Michael Romano [verfasserIn] |
---|
Format: |
E-Artikel |
---|---|
Sprache: |
Englisch |
Erschienen: |
2023 |
---|
Schlagwörter: |
---|
Übergeordnetes Werk: |
In: Physical Sciences Forum - MDPI AG, 2023, 7(2023), 1, p 32 |
---|---|
Übergeordnetes Werk: |
volume:7 ; year:2023 ; number:1, p 32 |
Links: |
---|
DOI / URN: |
10.3390/ECU2023-14072 |
---|
Katalog-ID: |
DOAJ094072329 |
---|
LEADER | 01000naa a22002652 4500 | ||
---|---|---|---|
001 | DOAJ094072329 | ||
003 | DE-627 | ||
005 | 20240413025221.0 | ||
007 | cr uuu---uuuuu | ||
008 | 240413s2023 xx |||||o 00| ||eng c | ||
024 | 7 | |a 10.3390/ECU2023-14072 |2 doi | |
035 | |a (DE-627)DOAJ094072329 | ||
035 | |a (DE-599)DOAJc8e23da195a9461fb2d2e1d8698bd8fd | ||
040 | |a DE-627 |b ger |c DE-627 |e rakwb | ||
041 | |a eng | ||
050 | 0 | |a T351-385 | |
050 | 0 | |a QD450-801 | |
100 | 0 | |a Michael Romano |e verfasserin |4 aut | |
245 | 1 | 0 | |a Constraining Star-Formation Driven Outflows in Local Dwarf Galaxies with <i<Herschel</i<<xref rid="fn1-psf-2287691" ref-type="fn"<†</xref< |
264 | 1 | |c 2023 | |
336 | |a Text |b txt |2 rdacontent | ||
337 | |a Computermedien |b c |2 rdamedia | ||
338 | |a Online-Ressource |b cr |2 rdacarrier | ||
520 | |a Galactic feedback (i.e., outflows) plays a fundamental role in regulating galaxy formation and evolution. We investigate the physical properties of galactic outflows in a sample of 29 local low-metallicity dwarf galaxies drawn from the Dwarf Galaxy Survey. We make use of Herschel/PACS archival data to detect outflows in the broad wings of observed [CII] 158 μm line profiles. We detect outflowing gas in 1/3 of the sample, and in the average galaxy population through line stacking. We find typical mass-loading factors (i.e., outflow efficiencies) of the order of unity. Outflow velocities are larger than the velocities required from gas to escape the gravitational potential of our targets, suggesting that a significant amount of gas and dust is brought out of their halos. Our results will be used as input for chemical models, posing new constraints on the processes of dust production/destruction in the interstellar medium of galaxies. | ||
650 | 4 | |a galaxies: dwarf | |
650 | 4 | |a galaxies: evolution | |
650 | 4 | |a galaxies: ISM | |
650 | 4 | |a galaxies: starburst | |
650 | 4 | |a ISM: jest and outflows | |
653 | 0 | |a Mechanical drawing. Engineering graphics | |
653 | 0 | |a Physical and theoretical chemistry | |
773 | 0 | 8 | |i In |t Physical Sciences Forum |d MDPI AG, 2023 |g 7(2023), 1, p 32 |w (DE-627)1870881796 |x 26739984 |7 nnns |
773 | 1 | 8 | |g volume:7 |g year:2023 |g number:1, p 32 |
856 | 4 | 0 | |u https://doi.org/10.3390/ECU2023-14072 |z kostenfrei |
856 | 4 | 0 | |u https://doaj.org/article/c8e23da195a9461fb2d2e1d8698bd8fd |z kostenfrei |
856 | 4 | 0 | |u https://www.mdpi.com/2673-9984/7/1/32 |z kostenfrei |
856 | 4 | 2 | |u https://doaj.org/toc/2673-9984 |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_31 | ||
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_2014 | ||
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 7 |j 2023 |e 1, p 32 |
author_variant |
m r mr |
---|---|
matchkey_str |
article:26739984:2023----::osriigtromtodieotlwilclwrglxewtieshlxer |
hierarchy_sort_str |
2023 |
callnumber-subject-code |
T |
publishDate |
2023 |
allfields |
10.3390/ECU2023-14072 doi (DE-627)DOAJ094072329 (DE-599)DOAJc8e23da195a9461fb2d2e1d8698bd8fd DE-627 ger DE-627 rakwb eng T351-385 QD450-801 Michael Romano verfasserin aut Constraining Star-Formation Driven Outflows in Local Dwarf Galaxies with <i<Herschel</i<<xref rid="fn1-psf-2287691" ref-type="fn"<†</xref< 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Galactic feedback (i.e., outflows) plays a fundamental role in regulating galaxy formation and evolution. We investigate the physical properties of galactic outflows in a sample of 29 local low-metallicity dwarf galaxies drawn from the Dwarf Galaxy Survey. We make use of Herschel/PACS archival data to detect outflows in the broad wings of observed [CII] 158 μm line profiles. We detect outflowing gas in 1/3 of the sample, and in the average galaxy population through line stacking. We find typical mass-loading factors (i.e., outflow efficiencies) of the order of unity. Outflow velocities are larger than the velocities required from gas to escape the gravitational potential of our targets, suggesting that a significant amount of gas and dust is brought out of their halos. Our results will be used as input for chemical models, posing new constraints on the processes of dust production/destruction in the interstellar medium of galaxies. galaxies: dwarf galaxies: evolution galaxies: ISM galaxies: starburst ISM: jest and outflows Mechanical drawing. Engineering graphics Physical and theoretical chemistry In Physical Sciences Forum MDPI AG, 2023 7(2023), 1, p 32 (DE-627)1870881796 26739984 nnns volume:7 year:2023 number:1, p 32 https://doi.org/10.3390/ECU2023-14072 kostenfrei https://doaj.org/article/c8e23da195a9461fb2d2e1d8698bd8fd kostenfrei https://www.mdpi.com/2673-9984/7/1/32 kostenfrei https://doaj.org/toc/2673-9984 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 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_2014 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 7 2023 1, p 32 |
spelling |
10.3390/ECU2023-14072 doi (DE-627)DOAJ094072329 (DE-599)DOAJc8e23da195a9461fb2d2e1d8698bd8fd DE-627 ger DE-627 rakwb eng T351-385 QD450-801 Michael Romano verfasserin aut Constraining Star-Formation Driven Outflows in Local Dwarf Galaxies with <i<Herschel</i<<xref rid="fn1-psf-2287691" ref-type="fn"<†</xref< 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Galactic feedback (i.e., outflows) plays a fundamental role in regulating galaxy formation and evolution. We investigate the physical properties of galactic outflows in a sample of 29 local low-metallicity dwarf galaxies drawn from the Dwarf Galaxy Survey. We make use of Herschel/PACS archival data to detect outflows in the broad wings of observed [CII] 158 μm line profiles. We detect outflowing gas in 1/3 of the sample, and in the average galaxy population through line stacking. We find typical mass-loading factors (i.e., outflow efficiencies) of the order of unity. Outflow velocities are larger than the velocities required from gas to escape the gravitational potential of our targets, suggesting that a significant amount of gas and dust is brought out of their halos. Our results will be used as input for chemical models, posing new constraints on the processes of dust production/destruction in the interstellar medium of galaxies. galaxies: dwarf galaxies: evolution galaxies: ISM galaxies: starburst ISM: jest and outflows Mechanical drawing. Engineering graphics Physical and theoretical chemistry In Physical Sciences Forum MDPI AG, 2023 7(2023), 1, p 32 (DE-627)1870881796 26739984 nnns volume:7 year:2023 number:1, p 32 https://doi.org/10.3390/ECU2023-14072 kostenfrei https://doaj.org/article/c8e23da195a9461fb2d2e1d8698bd8fd kostenfrei https://www.mdpi.com/2673-9984/7/1/32 kostenfrei https://doaj.org/toc/2673-9984 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 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_2014 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 7 2023 1, p 32 |
allfields_unstemmed |
10.3390/ECU2023-14072 doi (DE-627)DOAJ094072329 (DE-599)DOAJc8e23da195a9461fb2d2e1d8698bd8fd DE-627 ger DE-627 rakwb eng T351-385 QD450-801 Michael Romano verfasserin aut Constraining Star-Formation Driven Outflows in Local Dwarf Galaxies with <i<Herschel</i<<xref rid="fn1-psf-2287691" ref-type="fn"<†</xref< 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Galactic feedback (i.e., outflows) plays a fundamental role in regulating galaxy formation and evolution. We investigate the physical properties of galactic outflows in a sample of 29 local low-metallicity dwarf galaxies drawn from the Dwarf Galaxy Survey. We make use of Herschel/PACS archival data to detect outflows in the broad wings of observed [CII] 158 μm line profiles. We detect outflowing gas in 1/3 of the sample, and in the average galaxy population through line stacking. We find typical mass-loading factors (i.e., outflow efficiencies) of the order of unity. Outflow velocities are larger than the velocities required from gas to escape the gravitational potential of our targets, suggesting that a significant amount of gas and dust is brought out of their halos. Our results will be used as input for chemical models, posing new constraints on the processes of dust production/destruction in the interstellar medium of galaxies. galaxies: dwarf galaxies: evolution galaxies: ISM galaxies: starburst ISM: jest and outflows Mechanical drawing. Engineering graphics Physical and theoretical chemistry In Physical Sciences Forum MDPI AG, 2023 7(2023), 1, p 32 (DE-627)1870881796 26739984 nnns volume:7 year:2023 number:1, p 32 https://doi.org/10.3390/ECU2023-14072 kostenfrei https://doaj.org/article/c8e23da195a9461fb2d2e1d8698bd8fd kostenfrei https://www.mdpi.com/2673-9984/7/1/32 kostenfrei https://doaj.org/toc/2673-9984 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 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_2014 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 7 2023 1, p 32 |
allfieldsGer |
10.3390/ECU2023-14072 doi (DE-627)DOAJ094072329 (DE-599)DOAJc8e23da195a9461fb2d2e1d8698bd8fd DE-627 ger DE-627 rakwb eng T351-385 QD450-801 Michael Romano verfasserin aut Constraining Star-Formation Driven Outflows in Local Dwarf Galaxies with <i<Herschel</i<<xref rid="fn1-psf-2287691" ref-type="fn"<†</xref< 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Galactic feedback (i.e., outflows) plays a fundamental role in regulating galaxy formation and evolution. We investigate the physical properties of galactic outflows in a sample of 29 local low-metallicity dwarf galaxies drawn from the Dwarf Galaxy Survey. We make use of Herschel/PACS archival data to detect outflows in the broad wings of observed [CII] 158 μm line profiles. We detect outflowing gas in 1/3 of the sample, and in the average galaxy population through line stacking. We find typical mass-loading factors (i.e., outflow efficiencies) of the order of unity. Outflow velocities are larger than the velocities required from gas to escape the gravitational potential of our targets, suggesting that a significant amount of gas and dust is brought out of their halos. Our results will be used as input for chemical models, posing new constraints on the processes of dust production/destruction in the interstellar medium of galaxies. galaxies: dwarf galaxies: evolution galaxies: ISM galaxies: starburst ISM: jest and outflows Mechanical drawing. Engineering graphics Physical and theoretical chemistry In Physical Sciences Forum MDPI AG, 2023 7(2023), 1, p 32 (DE-627)1870881796 26739984 nnns volume:7 year:2023 number:1, p 32 https://doi.org/10.3390/ECU2023-14072 kostenfrei https://doaj.org/article/c8e23da195a9461fb2d2e1d8698bd8fd kostenfrei https://www.mdpi.com/2673-9984/7/1/32 kostenfrei https://doaj.org/toc/2673-9984 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 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_2014 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 7 2023 1, p 32 |
allfieldsSound |
10.3390/ECU2023-14072 doi (DE-627)DOAJ094072329 (DE-599)DOAJc8e23da195a9461fb2d2e1d8698bd8fd DE-627 ger DE-627 rakwb eng T351-385 QD450-801 Michael Romano verfasserin aut Constraining Star-Formation Driven Outflows in Local Dwarf Galaxies with <i<Herschel</i<<xref rid="fn1-psf-2287691" ref-type="fn"<†</xref< 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Galactic feedback (i.e., outflows) plays a fundamental role in regulating galaxy formation and evolution. We investigate the physical properties of galactic outflows in a sample of 29 local low-metallicity dwarf galaxies drawn from the Dwarf Galaxy Survey. We make use of Herschel/PACS archival data to detect outflows in the broad wings of observed [CII] 158 μm line profiles. We detect outflowing gas in 1/3 of the sample, and in the average galaxy population through line stacking. We find typical mass-loading factors (i.e., outflow efficiencies) of the order of unity. Outflow velocities are larger than the velocities required from gas to escape the gravitational potential of our targets, suggesting that a significant amount of gas and dust is brought out of their halos. Our results will be used as input for chemical models, posing new constraints on the processes of dust production/destruction in the interstellar medium of galaxies. galaxies: dwarf galaxies: evolution galaxies: ISM galaxies: starburst ISM: jest and outflows Mechanical drawing. Engineering graphics Physical and theoretical chemistry In Physical Sciences Forum MDPI AG, 2023 7(2023), 1, p 32 (DE-627)1870881796 26739984 nnns volume:7 year:2023 number:1, p 32 https://doi.org/10.3390/ECU2023-14072 kostenfrei https://doaj.org/article/c8e23da195a9461fb2d2e1d8698bd8fd kostenfrei https://www.mdpi.com/2673-9984/7/1/32 kostenfrei https://doaj.org/toc/2673-9984 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 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_2014 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 7 2023 1, p 32 |
language |
English |
source |
In Physical Sciences Forum 7(2023), 1, p 32 volume:7 year:2023 number:1, p 32 |
sourceStr |
In Physical Sciences Forum 7(2023), 1, p 32 volume:7 year:2023 number:1, p 32 |
format_phy_str_mv |
Article |
institution |
findex.gbv.de |
topic_facet |
galaxies: dwarf galaxies: evolution galaxies: ISM galaxies: starburst ISM: jest and outflows Mechanical drawing. Engineering graphics Physical and theoretical chemistry |
isfreeaccess_bool |
true |
container_title |
Physical Sciences Forum |
authorswithroles_txt_mv |
Michael Romano @@aut@@ |
publishDateDaySort_date |
2023-01-01T00:00:00Z |
hierarchy_top_id |
1870881796 |
id |
DOAJ094072329 |
language_de |
englisch |
fullrecord |
<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000naa a22002652 4500</leader><controlfield tag="001">DOAJ094072329</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20240413025221.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">240413s2023 xx |||||o 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.3390/ECU2023-14072</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)DOAJ094072329</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)DOAJc8e23da195a9461fb2d2e1d8698bd8fd</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">T351-385</subfield></datafield><datafield tag="050" ind1=" " ind2="0"><subfield code="a">QD450-801</subfield></datafield><datafield tag="100" ind1="0" ind2=" "><subfield code="a">Michael Romano</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Constraining Star-Formation Driven Outflows in Local Dwarf Galaxies with <i<Herschel</i<<xref rid="fn1-psf-2287691" ref-type="fn"<†</xref<</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2023</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">Galactic feedback (i.e., outflows) plays a fundamental role in regulating galaxy formation and evolution. We investigate the physical properties of galactic outflows in a sample of 29 local low-metallicity dwarf galaxies drawn from the Dwarf Galaxy Survey. We make use of Herschel/PACS archival data to detect outflows in the broad wings of observed [CII] 158 μm line profiles. We detect outflowing gas in 1/3 of the sample, and in the average galaxy population through line stacking. We find typical mass-loading factors (i.e., outflow efficiencies) of the order of unity. Outflow velocities are larger than the velocities required from gas to escape the gravitational potential of our targets, suggesting that a significant amount of gas and dust is brought out of their halos. Our results will be used as input for chemical models, posing new constraints on the processes of dust production/destruction in the interstellar medium of galaxies.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">galaxies: dwarf</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">galaxies: evolution</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">galaxies: ISM</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">galaxies: starburst</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">ISM: jest and outflows</subfield></datafield><datafield tag="653" ind1=" " ind2="0"><subfield code="a">Mechanical drawing. Engineering graphics</subfield></datafield><datafield tag="653" ind1=" " ind2="0"><subfield code="a">Physical and theoretical chemistry</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">In</subfield><subfield code="t">Physical Sciences Forum</subfield><subfield code="d">MDPI AG, 2023</subfield><subfield code="g">7(2023), 1, p 32</subfield><subfield code="w">(DE-627)1870881796</subfield><subfield code="x">26739984</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:7</subfield><subfield code="g">year:2023</subfield><subfield code="g">number:1, p 32</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://doi.org/10.3390/ECU2023-14072</subfield><subfield code="z">kostenfrei</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://doaj.org/article/c8e23da195a9461fb2d2e1d8698bd8fd</subfield><subfield code="z">kostenfrei</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://www.mdpi.com/2673-9984/7/1/32</subfield><subfield code="z">kostenfrei</subfield></datafield><datafield tag="856" ind1="4" ind2="2"><subfield code="u">https://doaj.org/toc/2673-9984</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_31</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_2014</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">7</subfield><subfield code="j">2023</subfield><subfield code="e">1, p 32</subfield></datafield></record></collection>
|
callnumber-first |
T - Technology |
author |
Michael Romano |
spellingShingle |
Michael Romano misc T351-385 misc QD450-801 misc galaxies: dwarf misc galaxies: evolution misc galaxies: ISM misc galaxies: starburst misc ISM: jest and outflows misc Mechanical drawing. Engineering graphics misc Physical and theoretical chemistry Constraining Star-Formation Driven Outflows in Local Dwarf Galaxies with <i<Herschel</i<<xref rid="fn1-psf-2287691" ref-type="fn"<†</xref< |
authorStr |
Michael Romano |
ppnlink_with_tag_str_mv |
@@773@@(DE-627)1870881796 |
format |
electronic Article |
delete_txt_mv |
keep |
author_role |
aut |
collection |
DOAJ |
remote_str |
true |
callnumber-label |
T351-385 |
illustrated |
Not Illustrated |
issn |
26739984 |
topic_title |
T351-385 QD450-801 Constraining Star-Formation Driven Outflows in Local Dwarf Galaxies with <i<Herschel</i<<xref rid="fn1-psf-2287691" ref-type="fn"<†</xref< galaxies: dwarf galaxies: evolution galaxies: ISM galaxies: starburst ISM: jest and outflows |
topic |
misc T351-385 misc QD450-801 misc galaxies: dwarf misc galaxies: evolution misc galaxies: ISM misc galaxies: starburst misc ISM: jest and outflows misc Mechanical drawing. Engineering graphics misc Physical and theoretical chemistry |
topic_unstemmed |
misc T351-385 misc QD450-801 misc galaxies: dwarf misc galaxies: evolution misc galaxies: ISM misc galaxies: starburst misc ISM: jest and outflows misc Mechanical drawing. Engineering graphics misc Physical and theoretical chemistry |
topic_browse |
misc T351-385 misc QD450-801 misc galaxies: dwarf misc galaxies: evolution misc galaxies: ISM misc galaxies: starburst misc ISM: jest and outflows misc Mechanical drawing. Engineering graphics misc Physical and theoretical chemistry |
format_facet |
Elektronische Aufsätze Aufsätze Elektronische Ressource |
format_main_str_mv |
Text Zeitschrift/Artikel |
carriertype_str_mv |
cr |
hierarchy_parent_title |
Physical Sciences Forum |
hierarchy_parent_id |
1870881796 |
hierarchy_top_title |
Physical Sciences Forum |
isfreeaccess_txt |
true |
familylinks_str_mv |
(DE-627)1870881796 |
title |
Constraining Star-Formation Driven Outflows in Local Dwarf Galaxies with <i<Herschel</i<<xref rid="fn1-psf-2287691" ref-type="fn"<†</xref< |
ctrlnum |
(DE-627)DOAJ094072329 (DE-599)DOAJc8e23da195a9461fb2d2e1d8698bd8fd |
title_full |
Constraining Star-Formation Driven Outflows in Local Dwarf Galaxies with <i<Herschel</i<<xref rid="fn1-psf-2287691" ref-type="fn"<†</xref< |
author_sort |
Michael Romano |
journal |
Physical Sciences Forum |
journalStr |
Physical Sciences Forum |
callnumber-first-code |
T |
lang_code |
eng |
isOA_bool |
true |
recordtype |
marc |
publishDateSort |
2023 |
contenttype_str_mv |
txt |
author_browse |
Michael Romano |
container_volume |
7 |
class |
T351-385 QD450-801 |
format_se |
Elektronische Aufsätze |
author-letter |
Michael Romano |
doi_str_mv |
10.3390/ECU2023-14072 |
title_sort |
constraining star-formation driven outflows in local dwarf galaxies with <i<herschel</i<<xref rid="fn1-psf-2287691" ref-type="fn"<†</xref< |
callnumber |
T351-385 |
title_auth |
Constraining Star-Formation Driven Outflows in Local Dwarf Galaxies with <i<Herschel</i<<xref rid="fn1-psf-2287691" ref-type="fn"<†</xref< |
abstract |
Galactic feedback (i.e., outflows) plays a fundamental role in regulating galaxy formation and evolution. We investigate the physical properties of galactic outflows in a sample of 29 local low-metallicity dwarf galaxies drawn from the Dwarf Galaxy Survey. We make use of Herschel/PACS archival data to detect outflows in the broad wings of observed [CII] 158 μm line profiles. We detect outflowing gas in 1/3 of the sample, and in the average galaxy population through line stacking. We find typical mass-loading factors (i.e., outflow efficiencies) of the order of unity. Outflow velocities are larger than the velocities required from gas to escape the gravitational potential of our targets, suggesting that a significant amount of gas and dust is brought out of their halos. Our results will be used as input for chemical models, posing new constraints on the processes of dust production/destruction in the interstellar medium of galaxies. |
abstractGer |
Galactic feedback (i.e., outflows) plays a fundamental role in regulating galaxy formation and evolution. We investigate the physical properties of galactic outflows in a sample of 29 local low-metallicity dwarf galaxies drawn from the Dwarf Galaxy Survey. We make use of Herschel/PACS archival data to detect outflows in the broad wings of observed [CII] 158 μm line profiles. We detect outflowing gas in 1/3 of the sample, and in the average galaxy population through line stacking. We find typical mass-loading factors (i.e., outflow efficiencies) of the order of unity. Outflow velocities are larger than the velocities required from gas to escape the gravitational potential of our targets, suggesting that a significant amount of gas and dust is brought out of their halos. Our results will be used as input for chemical models, posing new constraints on the processes of dust production/destruction in the interstellar medium of galaxies. |
abstract_unstemmed |
Galactic feedback (i.e., outflows) plays a fundamental role in regulating galaxy formation and evolution. We investigate the physical properties of galactic outflows in a sample of 29 local low-metallicity dwarf galaxies drawn from the Dwarf Galaxy Survey. We make use of Herschel/PACS archival data to detect outflows in the broad wings of observed [CII] 158 μm line profiles. We detect outflowing gas in 1/3 of the sample, and in the average galaxy population through line stacking. We find typical mass-loading factors (i.e., outflow efficiencies) of the order of unity. Outflow velocities are larger than the velocities required from gas to escape the gravitational potential of our targets, suggesting that a significant amount of gas and dust is brought out of their halos. Our results will be used as input for chemical models, posing new constraints on the processes of dust production/destruction in the interstellar medium of galaxies. |
collection_details |
GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 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_2014 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 32 |
title_short |
Constraining Star-Formation Driven Outflows in Local Dwarf Galaxies with <i<Herschel</i<<xref rid="fn1-psf-2287691" ref-type="fn"<†</xref< |
url |
https://doi.org/10.3390/ECU2023-14072 https://doaj.org/article/c8e23da195a9461fb2d2e1d8698bd8fd https://www.mdpi.com/2673-9984/7/1/32 https://doaj.org/toc/2673-9984 |
remote_bool |
true |
ppnlink |
1870881796 |
callnumber-subject |
T - General Technology |
mediatype_str_mv |
c |
isOA_txt |
true |
hochschulschrift_bool |
false |
doi_str |
10.3390/ECU2023-14072 |
callnumber-a |
T351-385 |
up_date |
2024-07-03T21:05:32.222Z |
_version_ |
1803593430832513024 |
fullrecord_marcxml |
<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000naa a22002652 4500</leader><controlfield tag="001">DOAJ094072329</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20240413025221.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">240413s2023 xx |||||o 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.3390/ECU2023-14072</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)DOAJ094072329</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)DOAJc8e23da195a9461fb2d2e1d8698bd8fd</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">T351-385</subfield></datafield><datafield tag="050" ind1=" " ind2="0"><subfield code="a">QD450-801</subfield></datafield><datafield tag="100" ind1="0" ind2=" "><subfield code="a">Michael Romano</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Constraining Star-Formation Driven Outflows in Local Dwarf Galaxies with <i<Herschel</i<<xref rid="fn1-psf-2287691" ref-type="fn"<†</xref<</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2023</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">Galactic feedback (i.e., outflows) plays a fundamental role in regulating galaxy formation and evolution. We investigate the physical properties of galactic outflows in a sample of 29 local low-metallicity dwarf galaxies drawn from the Dwarf Galaxy Survey. We make use of Herschel/PACS archival data to detect outflows in the broad wings of observed [CII] 158 μm line profiles. We detect outflowing gas in 1/3 of the sample, and in the average galaxy population through line stacking. We find typical mass-loading factors (i.e., outflow efficiencies) of the order of unity. Outflow velocities are larger than the velocities required from gas to escape the gravitational potential of our targets, suggesting that a significant amount of gas and dust is brought out of their halos. Our results will be used as input for chemical models, posing new constraints on the processes of dust production/destruction in the interstellar medium of galaxies.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">galaxies: dwarf</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">galaxies: evolution</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">galaxies: ISM</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">galaxies: starburst</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">ISM: jest and outflows</subfield></datafield><datafield tag="653" ind1=" " ind2="0"><subfield code="a">Mechanical drawing. Engineering graphics</subfield></datafield><datafield tag="653" ind1=" " ind2="0"><subfield code="a">Physical and theoretical chemistry</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">In</subfield><subfield code="t">Physical Sciences Forum</subfield><subfield code="d">MDPI AG, 2023</subfield><subfield code="g">7(2023), 1, p 32</subfield><subfield code="w">(DE-627)1870881796</subfield><subfield code="x">26739984</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:7</subfield><subfield code="g">year:2023</subfield><subfield code="g">number:1, p 32</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://doi.org/10.3390/ECU2023-14072</subfield><subfield code="z">kostenfrei</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://doaj.org/article/c8e23da195a9461fb2d2e1d8698bd8fd</subfield><subfield code="z">kostenfrei</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://www.mdpi.com/2673-9984/7/1/32</subfield><subfield code="z">kostenfrei</subfield></datafield><datafield tag="856" ind1="4" ind2="2"><subfield code="u">https://doaj.org/toc/2673-9984</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_31</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_2014</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">7</subfield><subfield code="j">2023</subfield><subfield code="e">1, p 32</subfield></datafield></record></collection>
|
score |
7.402897 |