The growth of bulges and discs in relatively HI-rich galaxies: indication from HI scaling relations

doi:10.1093/mnras/stz3622

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	The growth of bulges and discs in relatively HI-rich galaxies: indication from HI scaling relations
	Chen, Xinkai 1,2; Wang, Jing 3; Kong, Xu 1,2; Catinella, Barbara 4,5; Shao, Li 6; Mo, Houjun 7,8,9
刊名	MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
	2020-02-01
卷号	492 期号:2 页码:2393-2404
关键词	galaxies: evolution galaxies: ISM galaxies: structure
ISSN号	0035-8711
DOI	10.1093/mnras/stz3622
英文摘要	We study the relation between the properties of the bulge/disc components and the HI mass fraction of galaxies. We find that at fixed stellar mass, disc colours are correlated with the HI mass fraction, while bulge colours are not. The lack of a correlation between the bulge colour and the HI mass fraction is regardless whether the bulges are pseudo, or whether the galaxies host bars or are interacting with a neighbour. There is no strong correlation between the colours of the discs and bulges either. These results suggest that the current total amount of HI is closely related to the formation of discs, but does not necessarily fuel the formation of (pseudo) bulges in an efficient way. We do not find evidence for the star formation in the discs to be quenched by the bulges.
资助项目	Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D)[CE170100013] ; National Science Foundation of China (NSFC)[11421303] ; National Science Foundation of China (NSFC)[11433005] ; National Science Foundation of China (NSFC)[11721303] ; National Science Foundation of China (NSFC)[11973038] ; National Science Foundation of China (NSFC)[11991052] ; National Key R&D Program of China[2016YFA0400702] ; National Key R&D Program of China[2017YFA0402600] ; Alfred P. Sloan Foundation ; National Science Foundation ; U.S. Department of Energy ; National Aeronautics and Space Administration ; Japanese Monbukagakusho ; Max Planck Society ; Higher Education Funding Council for England ; American Museum of Natural History ; Astrophysical Institute Potsdam ; University of Basel ; University of Cambridge ; CaseWestern Reserve University ; University of Chicago ; Drexel University ; Fermilab ; Institute for Advanced Study ; Japan Participation Group ; Johns Hopkins University ; Joint Institute for Nuclear Astrophysics ; Kavli Institute for Particle Astrophysics and Cosmology ; Korean Scientist Group ; Chinese Academy of Sciences (LAMOST) ; Los Alamos National Laboratory ; MaxPlanck-Institute for Astronomy (MPIA) ; Max-Planck-Institute for Astrophysics (MPA) ; New Mexico State University ; Ohio State University ; University of Pittsburgh ; University of Portsmouth ; Princeton University ; United States Naval Observatory ; University of Washington
WOS关键词	ARECIBO SDSS SURVEY ; STAR-FORMATION ; SKY SURVEY ; SECULAR EVOLUTION ; CLASSICAL BULGES ; MASSIVE GALAXIES ; STELLAR MASS ; GAS INFLOW ; CATALOG ; PSEUDOBULGES
WOS研究方向	Astronomy & Astrophysics
语种	英语
出版者	OXFORD UNIV PRESS
WOS记录号	WOS:000512297600062
资助机构	Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D) ; Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D) ; National Science Foundation of China (NSFC) ; National Science Foundation of China (NSFC) ; National Key R&D Program of China ; National Key R&D Program of China ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; National Science Foundation ; National Science Foundation ; U.S. Department of Energy ; U.S. Department of Energy ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; Japanese Monbukagakusho ; Japanese Monbukagakusho ; Max Planck Society ; Max Planck Society ; Higher Education Funding Council for England ; Higher Education Funding Council for England ; American Museum of Natural History ; American Museum of Natural History ; Astrophysical Institute Potsdam ; Astrophysical Institute Potsdam ; University of Basel ; University of Basel ; University of Cambridge ; University of Cambridge ; CaseWestern Reserve University ; CaseWestern Reserve University ; University of Chicago ; University of Chicago ; Drexel University ; Drexel University ; Fermilab ; Fermilab ; Institute for Advanced Study ; Institute for Advanced Study ; Japan Participation Group ; Japan Participation Group ; Johns Hopkins University ; Johns Hopkins University ; Joint Institute for Nuclear Astrophysics ; Joint Institute for Nuclear Astrophysics ; Kavli Institute for Particle Astrophysics and Cosmology ; Kavli Institute for Particle Astrophysics and Cosmology ; Korean Scientist Group ; Korean Scientist Group ; Chinese Academy of Sciences (LAMOST) ; Chinese Academy of Sciences (LAMOST) ; Los Alamos National Laboratory ; Los Alamos National Laboratory ; MaxPlanck-Institute for Astronomy (MPIA) ; MaxPlanck-Institute for Astronomy (MPIA) ; Max-Planck-Institute for Astrophysics (MPA) ; Max-Planck-Institute for Astrophysics (MPA) ; New Mexico State University ; New Mexico State University ; Ohio State University ; Ohio State University ; University of Pittsburgh ; University of Pittsburgh ; University of Portsmouth ; University of Portsmouth ; Princeton University ; Princeton University ; United States Naval Observatory ; United States Naval Observatory ; University of Washington ; University of Washington ; Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D) ; Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D) ; National Science Foundation of China (NSFC) ; National Science Foundation of China (NSFC) ; National Key R&D Program of China ; National Key R&D Program of China ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; National Science Foundation ; National Science Foundation ; U.S. Department of Energy ; U.S. Department of Energy ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; Japanese Monbukagakusho ; Japanese Monbukagakusho ; Max Planck Society ; Max Planck Society ; Higher Education Funding Council for England ; Higher Education Funding Council for England ; American Museum of Natural History ; American Museum of Natural History ; Astrophysical Institute Potsdam ; Astrophysical Institute Potsdam ; University of Basel ; University of Basel ; University of Cambridge ; University of Cambridge ; CaseWestern Reserve University ; CaseWestern Reserve University ; University of Chicago ; University of Chicago ; Drexel University ; Drexel University ; Fermilab ; Fermilab ; Institute for Advanced Study ; Institute for Advanced Study ; Japan Participation Group ; Japan Participation Group ; Johns Hopkins University ; Johns Hopkins University ; Joint Institute for Nuclear Astrophysics ; Joint Institute for Nuclear Astrophysics ; Kavli Institute for Particle Astrophysics and Cosmology ; Kavli Institute for Particle Astrophysics and Cosmology ; Korean Scientist Group ; Korean Scientist Group ; Chinese Academy of Sciences (LAMOST) ; Chinese Academy of Sciences (LAMOST) ; Los Alamos National Laboratory ; Los Alamos National Laboratory ; MaxPlanck-Institute for Astronomy (MPIA) ; MaxPlanck-Institute for Astronomy (MPIA) ; Max-Planck-Institute for Astrophysics (MPA) ; Max-Planck-Institute for Astrophysics (MPA) ; New Mexico State University ; New Mexico State University ; Ohio State University ; Ohio State University ; University of Pittsburgh ; University of Pittsburgh ; University of Portsmouth ; University of Portsmouth ; Princeton University ; Princeton University ; United States Naval Observatory ; United States Naval Observatory ; University of Washington ; University of Washington ; Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D) ; Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D) ; National Science Foundation of China (NSFC) ; National Science Foundation of China (NSFC) ; National Key R&D Program of China ; National Key R&D Program of China ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; National Science Foundation ; National Science Foundation ; U.S. Department of Energy ; U.S. Department of Energy ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; Japanese Monbukagakusho ; Japanese Monbukagakusho ; Max Planck Society ; Max Planck Society ; Higher Education Funding Council for England ; Higher Education Funding Council for England ; American Museum of Natural History ; American Museum of Natural History ; Astrophysical Institute Potsdam ; Astrophysical Institute Potsdam ; University of Basel ; University of Basel ; University of Cambridge ; University of Cambridge ; CaseWestern Reserve University ; CaseWestern Reserve University ; University of Chicago ; University of Chicago ; Drexel University ; Drexel University ; Fermilab ; Fermilab ; Institute for Advanced Study ; Institute for Advanced Study ; Japan Participation Group ; Japan Participation Group ; Johns Hopkins University ; Johns Hopkins University ; Joint Institute for Nuclear Astrophysics ; Joint Institute for Nuclear Astrophysics ; Kavli Institute for Particle Astrophysics and Cosmology ; Kavli Institute for Particle Astrophysics and Cosmology ; Korean Scientist Group ; Korean Scientist Group ; Chinese Academy of Sciences (LAMOST) ; Chinese Academy of Sciences (LAMOST) ; Los Alamos National Laboratory ; Los Alamos National Laboratory ; MaxPlanck-Institute for Astronomy (MPIA) ; MaxPlanck-Institute for Astronomy (MPIA) ; Max-Planck-Institute for Astrophysics (MPA) ; Max-Planck-Institute for Astrophysics (MPA) ; New Mexico State University ; New Mexico State University ; Ohio State University ; Ohio State University ; University of Pittsburgh ; University of Pittsburgh ; University of Portsmouth ; University of Portsmouth ; Princeton University ; Princeton University ; United States Naval Observatory ; United States Naval Observatory ; University of Washington ; University of Washington ; Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D) ; Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D) ; National Science Foundation of China (NSFC) ; National Science Foundation of China (NSFC) ; National Key R&D Program of China ; National Key R&D Program of China ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; National Science Foundation ; National Science Foundation ; U.S. Department of Energy ; U.S. Department of Energy ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; Japanese Monbukagakusho ; Japanese Monbukagakusho ; Max Planck Society ; Max Planck Society ; Higher Education Funding Council for England ; Higher Education Funding Council for England ; American Museum of Natural History ; American Museum of Natural History ; Astrophysical Institute Potsdam ; Astrophysical Institute Potsdam ; University of Basel ; University of Basel ; University of Cambridge ; University of Cambridge ; CaseWestern Reserve University ; CaseWestern Reserve University ; University of Chicago ; University of Chicago ; Drexel University ; Drexel University ; Fermilab ; Fermilab ; Institute for Advanced Study ; Institute for Advanced Study ; Japan Participation Group ; Japan Participation Group ; Johns Hopkins University ; Johns Hopkins University ; Joint Institute for Nuclear Astrophysics ; Joint Institute for Nuclear Astrophysics ; Kavli Institute for Particle Astrophysics and Cosmology ; Kavli Institute for Particle Astrophysics and Cosmology ; Korean Scientist Group ; Korean Scientist Group ; Chinese Academy of Sciences (LAMOST) ; Chinese Academy of Sciences (LAMOST) ; Los Alamos National Laboratory ; Los Alamos National Laboratory ; MaxPlanck-Institute for Astronomy (MPIA) ; MaxPlanck-Institute for Astronomy (MPIA) ; Max-Planck-Institute for Astrophysics (MPA) ; Max-Planck-Institute for Astrophysics (MPA) ; New Mexico State University ; New Mexico State University ; Ohio State University ; Ohio State University ; University of Pittsburgh ; University of Pittsburgh ; University of Portsmouth ; University of Portsmouth ; Princeton University ; Princeton University ; United States Naval Observatory ; United States Naval Observatory ; University of Washington ; University of Washington
内容类型	期刊论文
源URL	[http://ir.bao.ac.cn/handle/114a11/54162]
专题	中国科学院国家天文台
通讯作者	Wang, Jing
作者单位	1.Univ Sci & Technol China, Dept Astron, CAS Key Lab Res Galaxies & Cosmol, Hefei 230026, Peoples R China 2.Univ Sci & Technol China, Sch Astron & Space Sci, Hefei 230026, Peoples R China 3.Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China 4.Univ Western Australia, Int Ctr Radio Astron Res, M468, Crawley, WA 6009, Australia 5.Australian Res Council, Ctr Excellence All Sky Astrophys 3 Dimens ASTRO 3, Sydney, NSW, Australia 6.Chinese Acad Sci, Natl Astron Observ, 20A Datun Rd, Beijing 100012, Peoples R China 7.Univ Massachusetts, Dept Astron, Amherst, MA 01003 USA 8.Tsinghua Univ, Tsinghua Ctr Astrophys, Beijing 100084, Peoples R China 9.Tsinghua Univ, Dept Phys, Beijing 100084, Peoples R China
推荐引用方式 GB/T 7714	Chen, Xinkai,Wang, Jing,Kong, Xu,et al. The growth of bulges and discs in relatively HI-rich galaxies: indication from HI scaling relations[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2020,492(2):2393-2404.
APA	Chen, Xinkai,Wang, Jing,Kong, Xu,Catinella, Barbara,Shao, Li,&Mo, Houjun.(2020).The growth of bulges and discs in relatively HI-rich galaxies: indication from HI scaling relations.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,492(2),2393-2404.
MLA	Chen, Xinkai,et al."The growth of bulges and discs in relatively HI-rich galaxies: indication from HI scaling relations".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 492.2(2020):2393-2404.