The SAMI Galaxy Survey: Observing the environmental quenching of star formation in GAMA groups
We explore the radial distribution of star formation in galaxies in the SAMI Galaxy Survey as a function of their Local Group environment. Using a sample of galaxies in groups (with halo masses less than ≃ 1014M⊙) from the Galaxy And Mass Assembly Survey, we find signatures of environmental quenchin...
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Online Access: | https://doi.org/10.1093/mnras/sty3258 https://hdl.handle.net/1959.7/uws:66836 |
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ftunivwestsyd:oai:researchdirect.westernsydney.edu.au:uws_66836 2023-05-15T18:11:32+02:00 The SAMI Galaxy Survey: Observing the environmental quenching of star formation in GAMA groups Schaefer, A. L. Croom, S. M. Scott, N. Brough, S. Allen, J. T. Bekki, K. Bland-Hawthorn, J. Bloom, J. V. Bryant, J. J. Cortese, L. Davies, L. J. M. Federrath, C. Fogarty, L. M. R. Green, A. W. Groves, B. Hopkins, Andrew M. (R20610) Konstantopoulos, I. S. López-Sánchez, A. R. Lawrence, J. S. McElroy, R. E. Medling, A. M. Owers, M. S. Pracy, M.B. Richards, S.N. Robotham, A.S.G. van de Sande, J. Tonini, C. Yi, S. K. 2019 print 20 https://doi.org/10.1093/mnras/sty3258 https://hdl.handle.net/1959.7/uws:66836 eng eng U.K., Oxford University Press Monthly Notices of the Royal Astronomical Society--0035-8711--1365-2966 Vol. 483 Issue. 3 No. pp: 2851-2870 XXXXXX - Unknown journal article 2019 ftunivwestsyd https://doi.org/10.1093/mnras/sty3258 2022-08-22T22:25:11Z We explore the radial distribution of star formation in galaxies in the SAMI Galaxy Survey as a function of their Local Group environment. Using a sample of galaxies in groups (with halo masses less than ≃ 1014M⊙) from the Galaxy And Mass Assembly Survey, we find signatures of environmental quenching in high-mass groups (MG ≥ 1012.5M⊙). The mean integrated specific star formation rate (sSFR) of star-forming galaxies in high-mass groups is lower than for galaxies in low-mass groups or those that are ungrouped, with Δlog(sSFR/yr-1) = 0.45 ± 0.07. This difference is seen at all galaxy stellar masses. In high-mass groups, starforming galaxies more massive than M∗ ∼ 1010M⊙ have centrally concentrated star formation. These galaxies also lie below the star formation main sequence, which suggests they may be undergoing outside-in quenching. Lower mass galaxies in high-mass groups do not show evidence of concentrated star formation. In groups less massive than MG = 1012.5M⊙, we do not observe these trends. In this regime, we find a modest correlation between centrally concentrated star formation and an enhancement in the total star formation rate, consistent with triggered star formation in these galaxies. Article in Journal/Newspaper sami University of Western Sydney (UWS): Research Direct Monthly Notices of the Royal Astronomical Society 483 3 2851 2870 |
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University of Western Sydney (UWS): Research Direct |
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ftunivwestsyd |
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English |
topic |
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XXXXXX - Unknown Schaefer, A. L. Croom, S. M. Scott, N. Brough, S. Allen, J. T. Bekki, K. Bland-Hawthorn, J. Bloom, J. V. Bryant, J. J. Cortese, L. Davies, L. J. M. Federrath, C. Fogarty, L. M. R. Green, A. W. Groves, B. Hopkins, Andrew M. (R20610) Konstantopoulos, I. S. López-Sánchez, A. R. Lawrence, J. S. McElroy, R. E. Medling, A. M. Owers, M. S. Pracy, M.B. Richards, S.N. Robotham, A.S.G. van de Sande, J. Tonini, C. Yi, S. K. The SAMI Galaxy Survey: Observing the environmental quenching of star formation in GAMA groups |
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description |
We explore the radial distribution of star formation in galaxies in the SAMI Galaxy Survey as a function of their Local Group environment. Using a sample of galaxies in groups (with halo masses less than ≃ 1014M⊙) from the Galaxy And Mass Assembly Survey, we find signatures of environmental quenching in high-mass groups (MG ≥ 1012.5M⊙). The mean integrated specific star formation rate (sSFR) of star-forming galaxies in high-mass groups is lower than for galaxies in low-mass groups or those that are ungrouped, with Δlog(sSFR/yr-1) = 0.45 ± 0.07. This difference is seen at all galaxy stellar masses. In high-mass groups, starforming galaxies more massive than M∗ ∼ 1010M⊙ have centrally concentrated star formation. These galaxies also lie below the star formation main sequence, which suggests they may be undergoing outside-in quenching. Lower mass galaxies in high-mass groups do not show evidence of concentrated star formation. In groups less massive than MG = 1012.5M⊙, we do not observe these trends. In this regime, we find a modest correlation between centrally concentrated star formation and an enhancement in the total star formation rate, consistent with triggered star formation in these galaxies. |
format |
Article in Journal/Newspaper |
author |
Schaefer, A. L. Croom, S. M. Scott, N. Brough, S. Allen, J. T. Bekki, K. Bland-Hawthorn, J. Bloom, J. V. Bryant, J. J. Cortese, L. Davies, L. J. M. Federrath, C. Fogarty, L. M. R. Green, A. W. Groves, B. Hopkins, Andrew M. (R20610) Konstantopoulos, I. S. López-Sánchez, A. R. Lawrence, J. S. McElroy, R. E. Medling, A. M. Owers, M. S. Pracy, M.B. Richards, S.N. Robotham, A.S.G. van de Sande, J. Tonini, C. Yi, S. K. |
author_facet |
Schaefer, A. L. Croom, S. M. Scott, N. Brough, S. Allen, J. T. Bekki, K. Bland-Hawthorn, J. Bloom, J. V. Bryant, J. J. Cortese, L. Davies, L. J. M. Federrath, C. Fogarty, L. M. R. Green, A. W. Groves, B. Hopkins, Andrew M. (R20610) Konstantopoulos, I. S. López-Sánchez, A. R. Lawrence, J. S. McElroy, R. E. Medling, A. M. Owers, M. S. Pracy, M.B. Richards, S.N. Robotham, A.S.G. van de Sande, J. Tonini, C. Yi, S. K. |
author_sort |
Schaefer, A. L. |
title |
The SAMI Galaxy Survey: Observing the environmental quenching of star formation in GAMA groups |
title_short |
The SAMI Galaxy Survey: Observing the environmental quenching of star formation in GAMA groups |
title_full |
The SAMI Galaxy Survey: Observing the environmental quenching of star formation in GAMA groups |
title_fullStr |
The SAMI Galaxy Survey: Observing the environmental quenching of star formation in GAMA groups |
title_full_unstemmed |
The SAMI Galaxy Survey: Observing the environmental quenching of star formation in GAMA groups |
title_sort |
sami galaxy survey: observing the environmental quenching of star formation in gama groups |
publisher |
U.K., Oxford University Press |
publishDate |
2019 |
url |
https://doi.org/10.1093/mnras/sty3258 https://hdl.handle.net/1959.7/uws:66836 |
genre |
sami |
genre_facet |
sami |
op_relation |
Monthly Notices of the Royal Astronomical Society--0035-8711--1365-2966 Vol. 483 Issue. 3 No. pp: 2851-2870 |
op_doi |
https://doi.org/10.1093/mnras/sty3258 |
container_title |
Monthly Notices of the Royal Astronomical Society |
container_volume |
483 |
container_issue |
3 |
container_start_page |
2851 |
op_container_end_page |
2870 |
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1766184182474604544 |