NAOC Open IR  > 星系宇宙学研究部
SDSS-IV MaNGA: environmental dependence of stellar age and metallicity gradients in nearby galaxies
Zheng, Zheng1; Wang, Huiyuan2; Ge, Junqiang1; Mao, Shude1,3,4,5; Li, Cheng3,4,6; Li, Ran1; Mo, Houjun3,4,7; Goddard, Daniel8; Bundy, Kevin; Li, Hongyu1,9; Nair, Preethi10; Lin, Lihwai11; Long, R. J.1,5; Riffel, Rogerio12,13; Thomas, Daniel8; Masters, Karen8; Bizyaev, Dmitry14,15,16; Brownstein, Joel R.17; Zhang, Kai18; Law, David R.19; Drory, Niv20; Roman Lopes, Alexandre21; Malanushenko, Olena14,15
2017-03-01
Source PublicationMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume465Issue:4Pages:4572-4588
AbstractWe present a study on the stellar age and metallicity distributions for 1105 galaxies using the STARLIGHT software on MaNGA (Mapping Nearby Galaxies at APO) integral field spectra. We derive age and metallicity gradients by fitting straight lines to the radial profiles, and explore their correlations with total stellar mass M-*, NUV - r colour and environments, as identified by both the large-scale structure (LSS) type and the local density. We find that the mean age and metallicity gradients are close to zero but slightly negative, which is consistent with the inside-out formation scenario. Within our sample, we find that both the age and metallicity gradients show weak or no correlation with either the LSS type or local density environment. In addition, we also study the environmental dependence of age and metallicity values at the effective radii. The age and metallicity values are highly correlated with M-* and NUV - r and are also dependent on LSS type as well as local density. Low-mass galaxies tend to be younger and have lower metallicity in low-density environments while high-mass galaxies are less affected by environment.
SubtypeArticle
KeywordGalaxies: Abundances Galaxies: Evolution Galaxies: Formation Galaxies: Statistics Galaxies: Stellar Content Galaxies: Structure
WOS HeadingsScience & Technology ; Physical Sciences
Funding OrganizationNational Astronomical Observatories, Chinese Academy of Sciences ; National Astronomical Observatories, Chinese Academy of Sciences ; Chinese Academy of Sciences(XDB09000000) ; Chinese Academy of Sciences(XDB09000000) ; NSFC(11333003 ; NSFC(11333003 ; National Key Basic Research Program of China(2015CB857004) ; National Key Basic Research Program of China(2015CB857004) ; World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan ; World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan ; JSPS KAKENHI(15K17603) ; JSPS KAKENHI(15K17603) ; STFC ; STFC ; CNPq ; CNPq ; FAPERGS ; FAPERGS ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; US Department of Energy Office of Science ; US Department of Energy Office of Science ; Centre for High-Performance Computing at the University of Utah ; Centre for High-Performance Computing at the University of Utah ; Brazilian Participation Group ; Brazilian Participation Group ; Carnegie Institution for Science ; Carnegie Institution for Science ; Carnegie Mellon University ; Carnegie Mellon University ; Chilean Participation Group ; Chilean Participation Group ; French Participation Group ; French Participation Group ; Harvard-Smithsonian Center for Astrophysics ; Harvard-Smithsonian Center for Astrophysics ; Instituto de Astrofsica de Canarias ; Instituto de Astrofsica de Canarias ; Johns Hopkins University ; Johns Hopkins University ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo ; Lawrence Berkeley National Laboratory ; Lawrence Berkeley National Laboratory ; Leibniz Institut fur Astrophysik Potsdam (AIP) ; Leibniz Institut fur Astrophysik Potsdam (AIP) ; Max-Planck-Institut fur Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fur Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fur Astrophysik (MPA Garching) ; Max-Planck-Institut fur Astrophysik (MPA Garching) ; Max-Planck-Institut fur Extraterrestrische Physik (MPE) ; Max-Planck-Institut fur Extraterrestrische Physik (MPE) ; National Astronomical Observatory of China ; National Astronomical Observatory of China ; New Mexico State University ; New Mexico State University ; New York University ; New York University ; University of Notre Dame ; University of Notre Dame ; Observatario Nacional/MCTI ; Observatario Nacional/MCTI ; Ohio State University ; Ohio State University ; Pennsylvania State University ; Pennsylvania State University ; Shanghai Astronomical Observatory ; Shanghai Astronomical Observatory ; United Kingdom Participation Group ; United Kingdom Participation Group ; Universidad Nacional Autonoma de Mexico ; Universidad Nacional Autonoma de Mexico ; University of Arizona ; University of Arizona ; University of Colorado Boulder ; University of Colorado Boulder ; University of Oxford ; University of Oxford ; University of Portsmouth ; University of Portsmouth ; University of Utah ; University of Utah ; University of Virginia ; University of Virginia ; University of Washington ; University of Washington ; University of Wisconsin ; University of Wisconsin ; Vanderbilt University ; Vanderbilt University ; Yale University ; Yale University ; (RSF 14-50-00043) ; (RSF 14-50-00043) ; 11390372 ; 11390372 ; 11173045 ; 11173045 ; 11233005 ; 11233005 ; 11325314 ; 11325314 ; 11320101002 ; 11320101002 ; 11522324 ; 11522324 ; 11421303) ; 11421303) ; National Astronomical Observatories, Chinese Academy of Sciences ; National Astronomical Observatories, Chinese Academy of Sciences ; Chinese Academy of Sciences(XDB09000000) ; Chinese Academy of Sciences(XDB09000000) ; NSFC(11333003 ; NSFC(11333003 ; National Key Basic Research Program of China(2015CB857004) ; National Key Basic Research Program of China(2015CB857004) ; World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan ; World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan ; JSPS KAKENHI(15K17603) ; JSPS KAKENHI(15K17603) ; STFC ; STFC ; CNPq ; CNPq ; FAPERGS ; FAPERGS ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; US Department of Energy Office of Science ; US Department of Energy Office of Science ; Centre for High-Performance Computing at the University of Utah ; Centre for High-Performance Computing at the University of Utah ; Brazilian Participation Group ; Brazilian Participation Group ; Carnegie Institution for Science ; Carnegie Institution for Science ; Carnegie Mellon University ; Carnegie Mellon University ; Chilean Participation Group ; Chilean Participation Group ; French Participation Group ; French Participation Group ; Harvard-Smithsonian Center for Astrophysics ; Harvard-Smithsonian Center for Astrophysics ; Instituto de Astrofsica de Canarias ; Instituto de Astrofsica de Canarias ; Johns Hopkins University ; Johns Hopkins University ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo ; Lawrence Berkeley National Laboratory ; Lawrence Berkeley National Laboratory ; Leibniz Institut fur Astrophysik Potsdam (AIP) ; Leibniz Institut fur Astrophysik Potsdam (AIP) ; Max-Planck-Institut fur Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fur Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fur Astrophysik (MPA Garching) ; Max-Planck-Institut fur Astrophysik (MPA Garching) ; Max-Planck-Institut fur Extraterrestrische Physik (MPE) ; Max-Planck-Institut fur Extraterrestrische Physik (MPE) ; National Astronomical Observatory of China ; National Astronomical Observatory of China ; New Mexico State University ; New Mexico State University ; New York University ; New York University ; University of Notre Dame ; University of Notre Dame ; Observatario Nacional/MCTI ; Observatario Nacional/MCTI ; Ohio State University ; Ohio State University ; Pennsylvania State University ; Pennsylvania State University ; Shanghai Astronomical Observatory ; Shanghai Astronomical Observatory ; United Kingdom Participation Group ; United Kingdom Participation Group ; Universidad Nacional Autonoma de Mexico ; Universidad Nacional Autonoma de Mexico ; University of Arizona ; University of Arizona ; University of Colorado Boulder ; University of Colorado Boulder ; University of Oxford ; University of Oxford ; University of Portsmouth ; University of Portsmouth ; University of Utah ; University of Utah ; University of Virginia ; University of Virginia ; University of Washington ; University of Washington ; University of Wisconsin ; University of Wisconsin ; Vanderbilt University ; Vanderbilt University ; Yale University ; Yale University ; (RSF 14-50-00043) ; (RSF 14-50-00043) ; 11390372 ; 11390372 ; 11173045 ; 11173045 ; 11233005 ; 11233005 ; 11325314 ; 11325314 ; 11320101002 ; 11320101002 ; 11522324 ; 11522324 ; 11421303) ; 11421303)
DOI10.1093/mnras/stw3030
WOS KeywordDIGITAL SKY SURVEY ; INTEGRAL-FIELD SPECTROSCOPY ; STAR-FORMATION HISTORIES ; DISK FORMATION SCENARIOS ; INITIAL MASS FUNCTION ; DARK-MATTER HALOES ; MEDIUM-DEEP SURVEY ; POPULATION GRADIENTS ; COLOR GRADIENTS ; ELLIPTIC GALAXIES
Indexed BySCI
Language英语
Funding OrganizationNational Astronomical Observatories, Chinese Academy of Sciences ; National Astronomical Observatories, Chinese Academy of Sciences ; Chinese Academy of Sciences(XDB09000000) ; Chinese Academy of Sciences(XDB09000000) ; NSFC(11333003 ; NSFC(11333003 ; National Key Basic Research Program of China(2015CB857004) ; National Key Basic Research Program of China(2015CB857004) ; World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan ; World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan ; JSPS KAKENHI(15K17603) ; JSPS KAKENHI(15K17603) ; STFC ; STFC ; CNPq ; CNPq ; FAPERGS ; FAPERGS ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; US Department of Energy Office of Science ; US Department of Energy Office of Science ; Centre for High-Performance Computing at the University of Utah ; Centre for High-Performance Computing at the University of Utah ; Brazilian Participation Group ; Brazilian Participation Group ; Carnegie Institution for Science ; Carnegie Institution for Science ; Carnegie Mellon University ; Carnegie Mellon University ; Chilean Participation Group ; Chilean Participation Group ; French Participation Group ; French Participation Group ; Harvard-Smithsonian Center for Astrophysics ; Harvard-Smithsonian Center for Astrophysics ; Instituto de Astrofsica de Canarias ; Instituto de Astrofsica de Canarias ; Johns Hopkins University ; Johns Hopkins University ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo ; Lawrence Berkeley National Laboratory ; Lawrence Berkeley National Laboratory ; Leibniz Institut fur Astrophysik Potsdam (AIP) ; Leibniz Institut fur Astrophysik Potsdam (AIP) ; Max-Planck-Institut fur Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fur Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fur Astrophysik (MPA Garching) ; Max-Planck-Institut fur Astrophysik (MPA Garching) ; Max-Planck-Institut fur Extraterrestrische Physik (MPE) ; Max-Planck-Institut fur Extraterrestrische Physik (MPE) ; National Astronomical Observatory of China ; National Astronomical Observatory of China ; New Mexico State University ; New Mexico State University ; New York University ; New York University ; University of Notre Dame ; University of Notre Dame ; Observatario Nacional/MCTI ; Observatario Nacional/MCTI ; Ohio State University ; Ohio State University ; Pennsylvania State University ; Pennsylvania State University ; Shanghai Astronomical Observatory ; Shanghai Astronomical Observatory ; United Kingdom Participation Group ; United Kingdom Participation Group ; Universidad Nacional Autonoma de Mexico ; Universidad Nacional Autonoma de Mexico ; University of Arizona ; University of Arizona ; University of Colorado Boulder ; University of Colorado Boulder ; University of Oxford ; University of Oxford ; University of Portsmouth ; University of Portsmouth ; University of Utah ; University of Utah ; University of Virginia ; University of Virginia ; University of Washington ; University of Washington ; University of Wisconsin ; University of Wisconsin ; Vanderbilt University ; Vanderbilt University ; Yale University ; Yale University ; (RSF 14-50-00043) ; (RSF 14-50-00043) ; 11390372 ; 11390372 ; 11173045 ; 11173045 ; 11233005 ; 11233005 ; 11325314 ; 11325314 ; 11320101002 ; 11320101002 ; 11522324 ; 11522324 ; 11421303) ; 11421303) ; National Astronomical Observatories, Chinese Academy of Sciences ; National Astronomical Observatories, Chinese Academy of Sciences ; Chinese Academy of Sciences(XDB09000000) ; Chinese Academy of Sciences(XDB09000000) ; NSFC(11333003 ; NSFC(11333003 ; National Key Basic Research Program of China(2015CB857004) ; National Key Basic Research Program of China(2015CB857004) ; World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan ; World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan ; JSPS KAKENHI(15K17603) ; JSPS KAKENHI(15K17603) ; STFC ; STFC ; CNPq ; CNPq ; FAPERGS ; FAPERGS ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; US Department of Energy Office of Science ; US Department of Energy Office of Science ; Centre for High-Performance Computing at the University of Utah ; Centre for High-Performance Computing at the University of Utah ; Brazilian Participation Group ; Brazilian Participation Group ; Carnegie Institution for Science ; Carnegie Institution for Science ; Carnegie Mellon University ; Carnegie Mellon University ; Chilean Participation Group ; Chilean Participation Group ; French Participation Group ; French Participation Group ; Harvard-Smithsonian Center for Astrophysics ; Harvard-Smithsonian Center for Astrophysics ; Instituto de Astrofsica de Canarias ; Instituto de Astrofsica de Canarias ; Johns Hopkins University ; Johns Hopkins University ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo ; Lawrence Berkeley National Laboratory ; Lawrence Berkeley National Laboratory ; Leibniz Institut fur Astrophysik Potsdam (AIP) ; Leibniz Institut fur Astrophysik Potsdam (AIP) ; Max-Planck-Institut fur Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fur Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fur Astrophysik (MPA Garching) ; Max-Planck-Institut fur Astrophysik (MPA Garching) ; Max-Planck-Institut fur Extraterrestrische Physik (MPE) ; Max-Planck-Institut fur Extraterrestrische Physik (MPE) ; National Astronomical Observatory of China ; National Astronomical Observatory of China ; New Mexico State University ; New Mexico State University ; New York University ; New York University ; University of Notre Dame ; University of Notre Dame ; Observatario Nacional/MCTI ; Observatario Nacional/MCTI ; Ohio State University ; Ohio State University ; Pennsylvania State University ; Pennsylvania State University ; Shanghai Astronomical Observatory ; Shanghai Astronomical Observatory ; United Kingdom Participation Group ; United Kingdom Participation Group ; Universidad Nacional Autonoma de Mexico ; Universidad Nacional Autonoma de Mexico ; University of Arizona ; University of Arizona ; University of Colorado Boulder ; University of Colorado Boulder ; University of Oxford ; University of Oxford ; University of Portsmouth ; University of Portsmouth ; University of Utah ; University of Utah ; University of Virginia ; University of Virginia ; University of Washington ; University of Washington ; University of Wisconsin ; University of Wisconsin ; Vanderbilt University ; Vanderbilt University ; Yale University ; Yale University ; (RSF 14-50-00043) ; (RSF 14-50-00043) ; 11390372 ; 11390372 ; 11173045 ; 11173045 ; 11233005 ; 11233005 ; 11325314 ; 11325314 ; 11320101002 ; 11320101002 ; 11522324 ; 11522324 ; 11421303) ; 11421303)
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000395170200059
Citation statistics
Cited Times:30[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/8264
Collection星系宇宙学研究部
Affiliation1.Chinese Acad Sci, Natl Astron Observ, A20 Datun Rd, Beijing 100012, Peoples R China
2.Univ Sci & Technol China, Dept Astron, Key Lab Res Galaxies & Cosmol, Hefei 230026, Anhui, Peoples R China
3.Tsinghua Univ, Tsinghua Ctr Astrophys, Beijing 100084, Peoples R China
4.Tsinghua Univ, Dept Phys, Beijing 100084, Peoples R China
5.Univ Manchester, Sch Phys & Astron, Jodrell Bank Ctr Astrophys, Oxford Rd, Manchester M13 9PL, Lancs, England
6.Chinese Acad Sci, Shanghai Astron Observ, Shanghai 200030, Peoples R China
7.Univ Massachusetts, Dept Astron, Amherst, MA 01003 USA
8.Univ Portsmouth, Inst Cosmol & Gravitat, Dennis Sciama Bldg, Portsmouth PO1 3FX, Hants, England
9.Univ Tokyo, Kavli IPMU WP, UTIAS, Kashiwa, Chiba 2778583, Japan
10.Univ Alabama, Tuscaloosa, AL 35487 USA
11.Acad Sinica, Inst Astron & Astrophys, Taipei 10617, Taiwan
12.Univ Fed Rio Grande do Sul, Inst Fis, Dept Astron, CP 15051, BR-91501970 Porto Alegre, RS, Brazil
13.Lab Interinst E Astron, Rua Gen Jose Cristino,77 Vasco da Gama, BR-20921400 Rio De Janeiro, Brazil
14.Apache Point Observ, POB 59, Sunspot, NM 88349 USA
15.New Mexico State Univ, POB 59, Sunspot, NM 88349 USA
16.Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Moscow 119991, Russia
17.Univ Utah, Salt Lake City, UT 84112 USA
18.Univ Kentucky, Lexington, KY 40506 USA
19.Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA
20.Univ Texas Austin, McDonald Observ, 1 Univ Stn, Austin, TX 78712 USA
21.Univ La Serena, Fac Ciencias, Dept Fis, Cisterns 1200, La Serena, Chile
Recommended Citation
GB/T 7714
Zheng, Zheng,Wang, Huiyuan,Ge, Junqiang,et al. SDSS-IV MaNGA: environmental dependence of stellar age and metallicity gradients in nearby galaxies[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2017,465(4):4572-4588.
APA Zheng, Zheng.,Wang, Huiyuan.,Ge, Junqiang.,Mao, Shude.,Li, Cheng.,...&Malanushenko, Olena.(2017).SDSS-IV MaNGA: environmental dependence of stellar age and metallicity gradients in nearby galaxies.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,465(4),4572-4588.
MLA Zheng, Zheng,et al."SDSS-IV MaNGA: environmental dependence of stellar age and metallicity gradients in nearby galaxies".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 465.4(2017):4572-4588.
Files in This Item:
There are no files associated with this item.
Related Services
Recommend this item
Bookmark
Usage statistics
Export to Endnote
Google Scholar
Similar articles in Google Scholar
[Zheng, Zheng]'s Articles
[Wang, Huiyuan]'s Articles
[Ge, Junqiang]'s Articles
Baidu academic
Similar articles in Baidu academic
[Zheng, Zheng]'s Articles
[Wang, Huiyuan]'s Articles
[Ge, Junqiang]'s Articles
Bing Scholar
Similar articles in Bing Scholar
[Zheng, Zheng]'s Articles
[Wang, Huiyuan]'s Articles
[Ge, Junqiang]'s Articles
Terms of Use
No data!
Social Bookmark/Share
All comments (0)
No comment.
 

Items in the repository are protected by copyright, with all rights reserved, unless otherwise indicated.