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SDSS-IV MaNGA: stellar population gradients as a function of galaxy environment
Goddard, D.1; Thomas, D.1; Maraston, C.1; Westfall, K.1; Etherington, J.1; Riffel, R.2,3; Mallmann, N. D.2,3; Zheng, Z.4; Argudo-Fernandez, M.5; Bershady, M.6; Bundy, K.7; Drory, N.8; Law, D.9; Yan, R.10; Wake, D.6,11; Weijmans, A.12; Bizyaev, D.13,14; Brownstein, J.15; Lane, R. R.16; Maiolino, R.17,18; Masters, K.1; Merrifield, M.19; Nitschelm, C.20; Pan, K.13; Roman-Lopes, A.21; Storchi-Bergmann, T.2,3
2017-02-11
Source PublicationMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume465Issue:1Pages:688-700
AbstractWe study the internal radial gradients of stellar population properties within 1.5 R-e and analyse the impact of galaxy environment. We use a representative sample of 721 galaxies with masses ranging between 10(9)M(circle dot) and 10(11.5)M(circle dot) from the SDSS-IV survey MaNGA. We split this sample by morphology into early-type and late-type galaxies. Using the full spectral fitting code FIREFLY, we derive the light and mass-weighted stellar population properties, age and metallicity, and calculate the gradients of these properties. We use three independent methods to quantify galaxy environment, namely the Nth nearest neighbour, the tidal strength parameter Q and distinguish between central and satellite galaxies. In our analysis, we find that early-type galaxies generally exhibit shallowlight-weighted age gradients in agreement with the literature and mass-weighted median age gradients tend to be slightly positive. Late-type galaxies, instead, have negative light-weighted age gradients. We detect negative metallicity gradients in both early-and late-type galaxies that correlate with galaxy mass, with the gradients being steeper and the correlation with mass being stronger in late-types. We find, however, that stellar population gradients, for both morphological classifications, have no significant correlation with galaxy environment for all three characterizations of environment. Our results suggest that galaxy mass is the main driver of stellar population gradients in both early and late-type galaxies, and any environmental dependence, if present at all, must be very subtle.
SubtypeArticle
KeywordSurveys Galaxies: Evolution Galaxies: Elliptical And Lenticular Galaxies: Formation Cd Galaxies: Spiral Galaxies: Stellar Content
WOS HeadingsScience & Technology ; Physical Sciences
Funding OrganizationSTFC PhD studentship ; STFC PhD studentship ; Leverhulme Early Career Fellowship ; Leverhulme Early Career Fellowship ; Institute of Cosmology of Gravitation ; Institute of Cosmology of Gravitation ; SEPNet ; SEPNet ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; US Department of Energy Office of Science ; US Department of Energy Office of Science ; Center for High-Performance Computing at the University of Utah ; Center 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 Astrofisica de Canarias ; Instituto de Astrofisica 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 fr Astrophysik Potsdam (AIP) ; Leibniz Institut fr Astrophysik Potsdam (AIP) ; Max-Planck-Institut fr Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fr Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fr Astrophysik (MPA Garching) ; Max-Planck-Institut fr Astrophysik (MPA Garching) ; Max-Planck-Institut fr Extraterrestrische Physik (MPE) ; Max-Planck-Institut fr 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 ; Observatrio Nacional/MCTI ; Observatrio 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 Autnoma de Mexico ; Universidad Nacional Autnoma 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 ; STFC PhD studentship ; STFC PhD studentship ; Leverhulme Early Career Fellowship ; Leverhulme Early Career Fellowship ; Institute of Cosmology of Gravitation ; Institute of Cosmology of Gravitation ; SEPNet ; SEPNet ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; US Department of Energy Office of Science ; US Department of Energy Office of Science ; Center for High-Performance Computing at the University of Utah ; Center 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 Astrofisica de Canarias ; Instituto de Astrofisica 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 fr Astrophysik Potsdam (AIP) ; Leibniz Institut fr Astrophysik Potsdam (AIP) ; Max-Planck-Institut fr Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fr Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fr Astrophysik (MPA Garching) ; Max-Planck-Institut fr Astrophysik (MPA Garching) ; Max-Planck-Institut fr Extraterrestrische Physik (MPE) ; Max-Planck-Institut fr 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 ; Observatrio Nacional/MCTI ; Observatrio 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 Autnoma de Mexico ; Universidad Nacional Autnoma 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
DOI10.1093/mnras/stw2719
WOS KeywordDIGITAL SKY SURVEY ; COLOR-MAGNITUDE RELATION ; INITIAL MASS FUNCTION ; LARGE-SCALE STRUCTURE ; CALIFA SURVEY ; DARK-MATTER ; BRIGHTEST CLUSTER ; SAURON PROJECT ; STAR-FORMATION ; DATA RELEASE
Indexed BySCI
Language英语
Funding OrganizationSTFC PhD studentship ; STFC PhD studentship ; Leverhulme Early Career Fellowship ; Leverhulme Early Career Fellowship ; Institute of Cosmology of Gravitation ; Institute of Cosmology of Gravitation ; SEPNet ; SEPNet ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; US Department of Energy Office of Science ; US Department of Energy Office of Science ; Center for High-Performance Computing at the University of Utah ; Center 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 Astrofisica de Canarias ; Instituto de Astrofisica 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 fr Astrophysik Potsdam (AIP) ; Leibniz Institut fr Astrophysik Potsdam (AIP) ; Max-Planck-Institut fr Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fr Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fr Astrophysik (MPA Garching) ; Max-Planck-Institut fr Astrophysik (MPA Garching) ; Max-Planck-Institut fr Extraterrestrische Physik (MPE) ; Max-Planck-Institut fr 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 ; Observatrio Nacional/MCTI ; Observatrio 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 Autnoma de Mexico ; Universidad Nacional Autnoma 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 ; STFC PhD studentship ; STFC PhD studentship ; Leverhulme Early Career Fellowship ; Leverhulme Early Career Fellowship ; Institute of Cosmology of Gravitation ; Institute of Cosmology of Gravitation ; SEPNet ; SEPNet ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; US Department of Energy Office of Science ; US Department of Energy Office of Science ; Center for High-Performance Computing at the University of Utah ; Center 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 Astrofisica de Canarias ; Instituto de Astrofisica 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 fr Astrophysik Potsdam (AIP) ; Leibniz Institut fr Astrophysik Potsdam (AIP) ; Max-Planck-Institut fr Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fr Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fr Astrophysik (MPA Garching) ; Max-Planck-Institut fr Astrophysik (MPA Garching) ; Max-Planck-Institut fr Extraterrestrische Physik (MPE) ; Max-Planck-Institut fr 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 ; Observatrio Nacional/MCTI ; Observatrio 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 Autnoma de Mexico ; Universidad Nacional Autnoma 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
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000393782000048
Citation statistics
Cited Times:25[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/8294
Collection星系宇宙学研究部
Affiliation1.Univ Portsmouth, Inst Cosmol & Gravitat, Burnaby Rd, Portsmouth PO1 3FX, Hants, England
2.Univ Fed Rio Grande do Sul, Inst Fis, Campus Vale, Porto Alegre, RS, Brazil
3.Lab Interinst E Astron, Rua Gen Jose Cristino,77 Vasco da Gama, Rio De Janeiro, Brazil
4.Chinese Acad Sci, Natl Astron Observ, A20 Datun Rd, Beijing 100012, Peoples R China
5.Univ Antofagasta, Fac Cs Basicas, Unidad Astron, Avda U Antofagasta, Antofagasta 02800, Chile
6.Univ Wisconsin, Dept Astron, 475 N Charter St, Madison, WI 53706 USA
7.Univ Tokyo, Inst Adv Study, Kavli InstitGute Phys & Math Universe WPI, Kashiwa, Chiba 2778583, Japan
8.Univ Texas Austin, Dept Astron, McDonald Observ, Univ Stn 1, Austin, TX 78712 USA
9.Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA
10.Univ Kentucky, Dept Phys & Astron, 505 Rose St, Lexington, KY 40506 USA
11.Open Univ, Dept Phys Sci, Milton Keynes, Bucks, England
12.Univ St Andrews, Sch Phys & Astron, St Andrews KY16 9SS, Fife, Scotland
13.Apache Point Observ, POB 59, Sunspot, NM 88349 USA
14.Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Moscow, Russia
15.Univ Utah, Dept Phys & Astron, 115 S 1400 E, Salt Lake City, UT 84112 USA
16.Pontificia Univ Catlica Chile, Inst Astrofis, Av Vicuna Mackenna 4860, Santiago 7820436, Chile
17.Univ Cambridge, Cavendish Astrophys, Cambridge CB3 0HE, England
18.Univ Cambridge, Kavli Inst Cosmol, Cambridge CB3 0HE, England
19.Univ Nottingham, Sch Phys & Astron, Univ Pk, Nottingham NG7 2RD, England
20.Univ Antofagasta, Unidad Astron, Ave Angamos 601, Antofagasta 1270300, Chile
21.Univ La Serena, Fac Ciencias, Dept Fis, La Serena 1200, Chile
Recommended Citation
GB/T 7714
Goddard, D.,Thomas, D.,Maraston, C.,et al. SDSS-IV MaNGA: stellar population gradients as a function of galaxy environment[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2017,465(1):688-700.
APA Goddard, D..,Thomas, D..,Maraston, C..,Westfall, K..,Etherington, J..,...&Storchi-Bergmann, T..(2017).SDSS-IV MaNGA: stellar population gradients as a function of galaxy environment.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,465(1),688-700.
MLA Goddard, D.,et al."SDSS-IV MaNGA: stellar population gradients as a function of galaxy environment".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 465.1(2017):688-700.
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