A SAMI and MaNGA view on the kinematics of star-forming galaxies
We investigate the physical connection between the growth of dispersionsupported stellar structures (e.g. classical bulges) and position of galaxies on the star forming main sequence (SFMS) at z~0. Combining the might of the SAMI and MaNGA galaxy IFS surveys, we measure the λRe spin parameter for 37...
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ftsmithonian:oai:figshare.com:article/14493949 2023-05-15T18:11:10+02:00 A SAMI and MaNGA view on the kinematics of star-forming galaxies Fraser-McKelvie, Amelia (10707235) Cortese, Luca (10707238) van de Sande, Jesse (5287960) 2021-04-26T00:00:00Z https://doi.org/10.5281/zenodo.4721522 unknown https://figshare.com/articles/poster/A_SAMI_and_MaNGA_view_on_the_kinematics_of_star-forming_galaxies/14493949 doi:10.5281/zenodo.4721522 CC BY 4.0 CC-BY Biophysics Medicine Microbiology Physiology Biotechnology Evolutionary Biology Ecology Cancer Computational Biology Biological Sciences not elsewhere classified Physical Sciences not elsewhere classified MaNGA galaxy IFS surveys kinematic properties SAMI PSF SFMS seeing-dominated IFS data Image Poster 2021 ftsmithonian https://doi.org/10.5281/zenodo.4721522 2021-05-05T17:22:40Z We investigate the physical connection between the growth of dispersionsupported stellar structures (e.g. classical bulges) and position of galaxies on the star forming main sequence (SFMS) at z~0. Combining the might of the SAMI and MaNGA galaxy IFS surveys, we measure the λRe spin parameter for 3781 galaxies with reliable stellar kinematics. After first confirming the importance of PSF corrections for seeing-dominated IFS data, we present the kinematic properties of galaxies above, below, and on the SFMS. Above log M*~10.5, we find tantalising evidence for an increase in the number of galaxies with dispersion-supported structures, suggesting a connection between bulge growth and the bending of the main sequence. Our results suggest that while a population of galaxies possessing some dispersion-supported structure is already present on the SFMS, further growth would be required after the galaxy has quenched to match the kinematic properties observed in passive galaxies at z~0. Still Image sami Unknown |
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op_collection_id |
ftsmithonian |
language |
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topic |
Biophysics Medicine Microbiology Physiology Biotechnology Evolutionary Biology Ecology Cancer Computational Biology Biological Sciences not elsewhere classified Physical Sciences not elsewhere classified MaNGA galaxy IFS surveys kinematic properties SAMI PSF SFMS seeing-dominated IFS data |
spellingShingle |
Biophysics Medicine Microbiology Physiology Biotechnology Evolutionary Biology Ecology Cancer Computational Biology Biological Sciences not elsewhere classified Physical Sciences not elsewhere classified MaNGA galaxy IFS surveys kinematic properties SAMI PSF SFMS seeing-dominated IFS data Fraser-McKelvie, Amelia (10707235) Cortese, Luca (10707238) van de Sande, Jesse (5287960) A SAMI and MaNGA view on the kinematics of star-forming galaxies |
topic_facet |
Biophysics Medicine Microbiology Physiology Biotechnology Evolutionary Biology Ecology Cancer Computational Biology Biological Sciences not elsewhere classified Physical Sciences not elsewhere classified MaNGA galaxy IFS surveys kinematic properties SAMI PSF SFMS seeing-dominated IFS data |
description |
We investigate the physical connection between the growth of dispersionsupported stellar structures (e.g. classical bulges) and position of galaxies on the star forming main sequence (SFMS) at z~0. Combining the might of the SAMI and MaNGA galaxy IFS surveys, we measure the λRe spin parameter for 3781 galaxies with reliable stellar kinematics. After first confirming the importance of PSF corrections for seeing-dominated IFS data, we present the kinematic properties of galaxies above, below, and on the SFMS. Above log M*~10.5, we find tantalising evidence for an increase in the number of galaxies with dispersion-supported structures, suggesting a connection between bulge growth and the bending of the main sequence. Our results suggest that while a population of galaxies possessing some dispersion-supported structure is already present on the SFMS, further growth would be required after the galaxy has quenched to match the kinematic properties observed in passive galaxies at z~0. |
format |
Still Image |
author |
Fraser-McKelvie, Amelia (10707235) Cortese, Luca (10707238) van de Sande, Jesse (5287960) |
author_facet |
Fraser-McKelvie, Amelia (10707235) Cortese, Luca (10707238) van de Sande, Jesse (5287960) |
author_sort |
Fraser-McKelvie, Amelia (10707235) |
title |
A SAMI and MaNGA view on the kinematics of star-forming galaxies |
title_short |
A SAMI and MaNGA view on the kinematics of star-forming galaxies |
title_full |
A SAMI and MaNGA view on the kinematics of star-forming galaxies |
title_fullStr |
A SAMI and MaNGA view on the kinematics of star-forming galaxies |
title_full_unstemmed |
A SAMI and MaNGA view on the kinematics of star-forming galaxies |
title_sort |
sami and manga view on the kinematics of star-forming galaxies |
publishDate |
2021 |
url |
https://doi.org/10.5281/zenodo.4721522 |
genre |
sami |
genre_facet |
sami |
op_relation |
https://figshare.com/articles/poster/A_SAMI_and_MaNGA_view_on_the_kinematics_of_star-forming_galaxies/14493949 doi:10.5281/zenodo.4721522 |
op_rights |
CC BY 4.0 |
op_rightsnorm |
CC-BY |
op_doi |
https://doi.org/10.5281/zenodo.4721522 |
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1766183864768659456 |