The SAMI Galaxy Survey:the contribution of different kinematic classes to the stellar mass function of nearby galaxies
We use the complete Sydney-AAO Multi-object Integral field spectrograph (SAMI) Galaxy Survey to determine the contribution of slow rotators (SRs), as well as different types of fast rotators (FRs), to the stellar mass function of galaxies in the local Universe. We use stellar kinematics not only to...
Published in: | Monthly Notices of the Royal Astronomical Society |
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Online Access: | https://researchers.mq.edu.au/en/publications/289ccca1-8b0b-43c3-94f1-5061e3d7b86b https://doi.org/10.1093/mnras/stz3042 http://www.scopus.com/inward/record.url?scp=85079669162&partnerID=8YFLogxK http://purl.org/au-research/grants/arc/CE170100013 http://purl.org/au-research/grants/arc/FT140100255 |
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ftmacquarieunicr:oai:https://researchers.mq.edu.au:publications/289ccca1-8b0b-43c3-94f1-5061e3d7b86b 2024-10-13T14:10:35+00:00 The SAMI Galaxy Survey:the contribution of different kinematic classes to the stellar mass function of nearby galaxies Guo, Kexin Cortese, Luca Obreschkow, Danail Catinella, Barbara van de Sande, Jesse Croom, Scott M. Brough, Sarah Sweet, Sarah Bryant, Julia J. Medling, Anne Bland-Hawthorn, Joss Owers, Matt Richards, Samuel N. 2020-01-01 https://researchers.mq.edu.au/en/publications/289ccca1-8b0b-43c3-94f1-5061e3d7b86b https://doi.org/10.1093/mnras/stz3042 http://www.scopus.com/inward/record.url?scp=85079669162&partnerID=8YFLogxK http://purl.org/au-research/grants/arc/CE170100013 http://purl.org/au-research/grants/arc/FT140100255 eng eng info:eu-repo/semantics/closedAccess Guo , K , Cortese , L , Obreschkow , D , Catinella , B , van de Sande , J , Croom , S M , Brough , S , Sweet , S , Bryant , J J , Medling , A , Bland-Hawthorn , J , Owers , M & Richards , S N 2020 , ' The SAMI Galaxy Survey : the contribution of different kinematic classes to the stellar mass function of nearby galaxies ' , Monthly Notices of the Royal Astronomical Society , vol. 491 , no. 1 , pp. 773-781 . https://doi.org/10.1093/mnras/stz3042 Galaxies: abundances Galaxies: kinematics and dynamics Galaxies: stellar content article 2020 ftmacquarieunicr https://doi.org/10.1093/mnras/stz3042 2024-10-03T00:23:12Z We use the complete Sydney-AAO Multi-object Integral field spectrograph (SAMI) Galaxy Survey to determine the contribution of slow rotators (SRs), as well as different types of fast rotators (FRs), to the stellar mass function of galaxies in the local Universe. We use stellar kinematics not only to discriminate between fast and SRs, but also to distinguish between dynamically cold systems (i.e. consistent with intrinsic axis ratios <0.3) and systems including a prominent dispersion-supported bulge. We show that FRs account for more than 80 per cent of the stellar mass budget of nearby galaxies, confirming that their number density overwhelms that of SRs at almost all masses from 10 9 to 10 11.5 M ☉ . Most importantly, dynamically cold discs contribute to at least 25 per cent of the stellar mass budget of the local Universe, significantly higher than what is estimated from visual morphology alone. For stellar masses up to 10 10.5 M ☉ , this class makes up >= 30 per cent of the galaxy population in each stellar mass bin. The fact that many galaxies that are visually classified as having two-components have stellar spin consistent with dynamically cold discs suggests that the inner component is either rotationally dominated (e.g. bar, pseudo-bulge) or has little effect on the global stellar kinematics of galaxies. Article in Journal/Newspaper sami Macquarie University Research Portal Monthly Notices of the Royal Astronomical Society |
institution |
Open Polar |
collection |
Macquarie University Research Portal |
op_collection_id |
ftmacquarieunicr |
language |
English |
topic |
Galaxies: abundances Galaxies: kinematics and dynamics Galaxies: stellar content |
spellingShingle |
Galaxies: abundances Galaxies: kinematics and dynamics Galaxies: stellar content Guo, Kexin Cortese, Luca Obreschkow, Danail Catinella, Barbara van de Sande, Jesse Croom, Scott M. Brough, Sarah Sweet, Sarah Bryant, Julia J. Medling, Anne Bland-Hawthorn, Joss Owers, Matt Richards, Samuel N. The SAMI Galaxy Survey:the contribution of different kinematic classes to the stellar mass function of nearby galaxies |
topic_facet |
Galaxies: abundances Galaxies: kinematics and dynamics Galaxies: stellar content |
description |
We use the complete Sydney-AAO Multi-object Integral field spectrograph (SAMI) Galaxy Survey to determine the contribution of slow rotators (SRs), as well as different types of fast rotators (FRs), to the stellar mass function of galaxies in the local Universe. We use stellar kinematics not only to discriminate between fast and SRs, but also to distinguish between dynamically cold systems (i.e. consistent with intrinsic axis ratios <0.3) and systems including a prominent dispersion-supported bulge. We show that FRs account for more than 80 per cent of the stellar mass budget of nearby galaxies, confirming that their number density overwhelms that of SRs at almost all masses from 10 9 to 10 11.5 M ☉ . Most importantly, dynamically cold discs contribute to at least 25 per cent of the stellar mass budget of the local Universe, significantly higher than what is estimated from visual morphology alone. For stellar masses up to 10 10.5 M ☉ , this class makes up >= 30 per cent of the galaxy population in each stellar mass bin. The fact that many galaxies that are visually classified as having two-components have stellar spin consistent with dynamically cold discs suggests that the inner component is either rotationally dominated (e.g. bar, pseudo-bulge) or has little effect on the global stellar kinematics of galaxies. |
format |
Article in Journal/Newspaper |
author |
Guo, Kexin Cortese, Luca Obreschkow, Danail Catinella, Barbara van de Sande, Jesse Croom, Scott M. Brough, Sarah Sweet, Sarah Bryant, Julia J. Medling, Anne Bland-Hawthorn, Joss Owers, Matt Richards, Samuel N. |
author_facet |
Guo, Kexin Cortese, Luca Obreschkow, Danail Catinella, Barbara van de Sande, Jesse Croom, Scott M. Brough, Sarah Sweet, Sarah Bryant, Julia J. Medling, Anne Bland-Hawthorn, Joss Owers, Matt Richards, Samuel N. |
author_sort |
Guo, Kexin |
title |
The SAMI Galaxy Survey:the contribution of different kinematic classes to the stellar mass function of nearby galaxies |
title_short |
The SAMI Galaxy Survey:the contribution of different kinematic classes to the stellar mass function of nearby galaxies |
title_full |
The SAMI Galaxy Survey:the contribution of different kinematic classes to the stellar mass function of nearby galaxies |
title_fullStr |
The SAMI Galaxy Survey:the contribution of different kinematic classes to the stellar mass function of nearby galaxies |
title_full_unstemmed |
The SAMI Galaxy Survey:the contribution of different kinematic classes to the stellar mass function of nearby galaxies |
title_sort |
sami galaxy survey:the contribution of different kinematic classes to the stellar mass function of nearby galaxies |
publishDate |
2020 |
url |
https://researchers.mq.edu.au/en/publications/289ccca1-8b0b-43c3-94f1-5061e3d7b86b https://doi.org/10.1093/mnras/stz3042 http://www.scopus.com/inward/record.url?scp=85079669162&partnerID=8YFLogxK http://purl.org/au-research/grants/arc/CE170100013 http://purl.org/au-research/grants/arc/FT140100255 |
genre |
sami |
genre_facet |
sami |
op_source |
Guo , K , Cortese , L , Obreschkow , D , Catinella , B , van de Sande , J , Croom , S M , Brough , S , Sweet , S , Bryant , J J , Medling , A , Bland-Hawthorn , J , Owers , M & Richards , S N 2020 , ' The SAMI Galaxy Survey : the contribution of different kinematic classes to the stellar mass function of nearby galaxies ' , Monthly Notices of the Royal Astronomical Society , vol. 491 , no. 1 , pp. 773-781 . https://doi.org/10.1093/mnras/stz3042 |
op_rights |
info:eu-repo/semantics/closedAccess |
op_doi |
https://doi.org/10.1093/mnras/stz3042 |
container_title |
Monthly Notices of the Royal Astronomical Society |
_version_ |
1812817899860000768 |