Star-forming, rotating spheroidal galaxies in the GAMA and SAMI Surveys
The Galaxy And Mass Assembly (GAMA) survey has morphologically identified a class of “Little Blue Spheroid” (LBS) galaxies whose relationship to other classes of galaxies we now examine in detail. Considering a sample of 868 LBSs, we find that such galaxies display similar but not identical colours,...
Published in: | Monthly Notices of the Royal Astronomical Society |
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Online Access: | https://research-portal.st-andrews.ac.uk/en/researchoutput/starforming-rotating-spheroidal-galaxies-in-the-gama-and-sami-surveys(65d3d335-5e3b-4f2f-8bca-361051b6c4e0).html https://doi.org/10.1093/mnras/stz2237 https://research-repository.st-andrews.ac.uk/bitstream/10023/18424/1/Moffett_2019_MNRAS_Star_forming_AAM.pdf |
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ftunstandrewcris:oai:research-portal.st-andrews.ac.uk:publications/65d3d335-5e3b-4f2f-8bca-361051b6c4e0 2024-06-23T07:56:32+00:00 Star-forming, rotating spheroidal galaxies in the GAMA and SAMI Surveys Moffett, Amanda J Phillipps, Steven Robotham, Aaron S G Driver, Simon P Bremer, Malcolm N Cortese, Luca Wong, O Ivy Brough, Sarah Brown, Michael J I Bryant, Julia J Conselice, Christopher J Croom, Scott M George, Koshy Goldstein, Greg Goodwin, Michael Holwerda, Benne W Hopkins, Andrew M Konstantopoulos, Iraklis S Lawrence, Jon S Lorente, Nuria P F Medling, Anne M Owers, Matt S Pimbblet, Kevin A Richards, Samuel N Sweet, Sarah M Van De Sande, Jesse 2019-10 application/pdf https://research-portal.st-andrews.ac.uk/en/researchoutput/starforming-rotating-spheroidal-galaxies-in-the-gama-and-sami-surveys(65d3d335-5e3b-4f2f-8bca-361051b6c4e0).html https://doi.org/10.1093/mnras/stz2237 https://research-repository.st-andrews.ac.uk/bitstream/10023/18424/1/Moffett_2019_MNRAS_Star_forming_AAM.pdf eng eng https://research-portal.st-andrews.ac.uk/en/researchoutput/starforming-rotating-spheroidal-galaxies-in-the-gama-and-sami-surveys(65d3d335-5e3b-4f2f-8bca-361051b6c4e0).html info:eu-repo/semantics/openAccess Moffett , A J , Phillipps , S , Robotham , A S G , Driver , S P , Bremer , M N , Cortese , L , Wong , O I , Brough , S , Brown , M J I , Bryant , J J , Conselice , C J , Croom , S M , George , K , Goldstein , G , Goodwin , M , Holwerda , B W , Hopkins , A M , Konstantopoulos , I S , Lawrence , J S , Lorente , N P F , Medling , A M , Owers , M S , Pimbblet , K A , Richards , S N , Sweet , S M & Van De Sande , J 2019 , ' Star-forming, rotating spheroidal galaxies in the GAMA and SAMI Surveys ' , Monthly Notices of the Royal Astronomical Society , vol. 489 , no. 2 , pp. 2830–2843 . https://doi.org/10.1093/mnras/stz2237 Surveys Galaxies: dwarf Galaxies: structure Galaxies: fundamental paramaters article 2019 ftunstandrewcris https://doi.org/10.1093/mnras/stz2237 2024-06-13T01:06:44Z The Galaxy And Mass Assembly (GAMA) survey has morphologically identified a class of “Little Blue Spheroid” (LBS) galaxies whose relationship to other classes of galaxies we now examine in detail. Considering a sample of 868 LBSs, we find that such galaxies display similar but not identical colours, specific star formation rates, stellar population ages, mass-to-light ratios, and metallicities to Sd-Irr galaxies. We also find that LBSs typically occupy environments of even lower density than those of Sd-Irr galaxies, where ∼65% of LBS galaxies live in isolation. Using deep, high-resolution imaging from VST KiDS and the new Bayesian, two-dimensional galaxy profile modeling code PROFIT, we further examine the detailed structure of LBSs and find that their Sérsic indices, sizes, and axial ratios are compatible with those of low-mass elliptical galaxies. We then examine SAMI Galaxy survey integral field emission line kinematics for a subset of 62 LBSs and find that the majority (42) of these galaxies display ordered rotation with the remainder displaying disturbed/non-ordered dynamics. Finally, we consider potential evolutionary scenarios for a population with this unusual combination of properties, concluding that LBSs are likely formed by a mixture of merger and accretion processes still recently active in low-redshift dwarf populations. We also infer that if LBS-like galaxies were subjected to quenching in a rich environment, they would plausibly resemble cluster dwarf ellipticals. Article in Journal/Newspaper sami University of St Andrews: Research Portal Monthly Notices of the Royal Astronomical Society 489 2 2830 2843 |
institution |
Open Polar |
collection |
University of St Andrews: Research Portal |
op_collection_id |
ftunstandrewcris |
language |
English |
topic |
Surveys Galaxies: dwarf Galaxies: structure Galaxies: fundamental paramaters |
spellingShingle |
Surveys Galaxies: dwarf Galaxies: structure Galaxies: fundamental paramaters Moffett, Amanda J Phillipps, Steven Robotham, Aaron S G Driver, Simon P Bremer, Malcolm N Cortese, Luca Wong, O Ivy Brough, Sarah Brown, Michael J I Bryant, Julia J Conselice, Christopher J Croom, Scott M George, Koshy Goldstein, Greg Goodwin, Michael Holwerda, Benne W Hopkins, Andrew M Konstantopoulos, Iraklis S Lawrence, Jon S Lorente, Nuria P F Medling, Anne M Owers, Matt S Pimbblet, Kevin A Richards, Samuel N Sweet, Sarah M Van De Sande, Jesse Star-forming, rotating spheroidal galaxies in the GAMA and SAMI Surveys |
topic_facet |
Surveys Galaxies: dwarf Galaxies: structure Galaxies: fundamental paramaters |
description |
The Galaxy And Mass Assembly (GAMA) survey has morphologically identified a class of “Little Blue Spheroid” (LBS) galaxies whose relationship to other classes of galaxies we now examine in detail. Considering a sample of 868 LBSs, we find that such galaxies display similar but not identical colours, specific star formation rates, stellar population ages, mass-to-light ratios, and metallicities to Sd-Irr galaxies. We also find that LBSs typically occupy environments of even lower density than those of Sd-Irr galaxies, where ∼65% of LBS galaxies live in isolation. Using deep, high-resolution imaging from VST KiDS and the new Bayesian, two-dimensional galaxy profile modeling code PROFIT, we further examine the detailed structure of LBSs and find that their Sérsic indices, sizes, and axial ratios are compatible with those of low-mass elliptical galaxies. We then examine SAMI Galaxy survey integral field emission line kinematics for a subset of 62 LBSs and find that the majority (42) of these galaxies display ordered rotation with the remainder displaying disturbed/non-ordered dynamics. Finally, we consider potential evolutionary scenarios for a population with this unusual combination of properties, concluding that LBSs are likely formed by a mixture of merger and accretion processes still recently active in low-redshift dwarf populations. We also infer that if LBS-like galaxies were subjected to quenching in a rich environment, they would plausibly resemble cluster dwarf ellipticals. |
format |
Article in Journal/Newspaper |
author |
Moffett, Amanda J Phillipps, Steven Robotham, Aaron S G Driver, Simon P Bremer, Malcolm N Cortese, Luca Wong, O Ivy Brough, Sarah Brown, Michael J I Bryant, Julia J Conselice, Christopher J Croom, Scott M George, Koshy Goldstein, Greg Goodwin, Michael Holwerda, Benne W Hopkins, Andrew M Konstantopoulos, Iraklis S Lawrence, Jon S Lorente, Nuria P F Medling, Anne M Owers, Matt S Pimbblet, Kevin A Richards, Samuel N Sweet, Sarah M Van De Sande, Jesse |
author_facet |
Moffett, Amanda J Phillipps, Steven Robotham, Aaron S G Driver, Simon P Bremer, Malcolm N Cortese, Luca Wong, O Ivy Brough, Sarah Brown, Michael J I Bryant, Julia J Conselice, Christopher J Croom, Scott M George, Koshy Goldstein, Greg Goodwin, Michael Holwerda, Benne W Hopkins, Andrew M Konstantopoulos, Iraklis S Lawrence, Jon S Lorente, Nuria P F Medling, Anne M Owers, Matt S Pimbblet, Kevin A Richards, Samuel N Sweet, Sarah M Van De Sande, Jesse |
author_sort |
Moffett, Amanda J |
title |
Star-forming, rotating spheroidal galaxies in the GAMA and SAMI Surveys |
title_short |
Star-forming, rotating spheroidal galaxies in the GAMA and SAMI Surveys |
title_full |
Star-forming, rotating spheroidal galaxies in the GAMA and SAMI Surveys |
title_fullStr |
Star-forming, rotating spheroidal galaxies in the GAMA and SAMI Surveys |
title_full_unstemmed |
Star-forming, rotating spheroidal galaxies in the GAMA and SAMI Surveys |
title_sort |
star-forming, rotating spheroidal galaxies in the gama and sami surveys |
publishDate |
2019 |
url |
https://research-portal.st-andrews.ac.uk/en/researchoutput/starforming-rotating-spheroidal-galaxies-in-the-gama-and-sami-surveys(65d3d335-5e3b-4f2f-8bca-361051b6c4e0).html https://doi.org/10.1093/mnras/stz2237 https://research-repository.st-andrews.ac.uk/bitstream/10023/18424/1/Moffett_2019_MNRAS_Star_forming_AAM.pdf |
genre |
sami |
genre_facet |
sami |
op_source |
Moffett , A J , Phillipps , S , Robotham , A S G , Driver , S P , Bremer , M N , Cortese , L , Wong , O I , Brough , S , Brown , M J I , Bryant , J J , Conselice , C J , Croom , S M , George , K , Goldstein , G , Goodwin , M , Holwerda , B W , Hopkins , A M , Konstantopoulos , I S , Lawrence , J S , Lorente , N P F , Medling , A M , Owers , M S , Pimbblet , K A , Richards , S N , Sweet , S M & Van De Sande , J 2019 , ' Star-forming, rotating spheroidal galaxies in the GAMA and SAMI Surveys ' , Monthly Notices of the Royal Astronomical Society , vol. 489 , no. 2 , pp. 2830–2843 . https://doi.org/10.1093/mnras/stz2237 |
op_relation |
https://research-portal.st-andrews.ac.uk/en/researchoutput/starforming-rotating-spheroidal-galaxies-in-the-gama-and-sami-surveys(65d3d335-5e3b-4f2f-8bca-361051b6c4e0).html |
op_rights |
info:eu-repo/semantics/openAccess |
op_doi |
https://doi.org/10.1093/mnras/stz2237 |
container_title |
Monthly Notices of the Royal Astronomical Society |
container_volume |
489 |
container_issue |
2 |
container_start_page |
2830 |
op_container_end_page |
2843 |
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1802649678111571968 |