The SAMI Galaxy Survey: Global stellar populations on the size-mass plane

Nicholas Scott, S. Brough, Scott M. Croom, Roger L. Davies, Jesse van de Sande, J. T. Allen, Joss Bland-Hawthorn, Julia J. Bryant, Luca Cortese, Francesco D'Eugenio, Christoph Federrath, Ignacio Ferreras, Michael Goodwin, Brent Groves, Iraklis Konstantopoulos, Jon S. Lawrence, Anne M. Medling, Amanda J. Moffett, Matt S. Owers, Samuel RichardsA. S.G. Robotham, Chiara Tonini, Sukyoung K. Yi

Research output: Contribution to journalArticle

16 Citations (Scopus)

Abstract

We present an analysis of the global stellar populations of galaxies in the SAMI (Sydney- AAO Multi-object Integral field spectrograph) Galaxy Survey. Our sample consists of 1319 galaxies spanning four orders of magnitude in stellar mass and includes all morphologies and environments. We derive luminosity-weighted, single stellar population equivalent stellar ages, metallicities and alpha enhancements from spectra integrated within one effective radius apertures. Variations in galaxy size explain the majority of the scatter in the age-mass and metallicity-mass relations. Stellar populations vary systematically in the plane of galaxy size and stellar mass, such that galaxies with high stellar surface mass density are older, more metal rich and alpha enhanced than less dense galaxies. Galaxies with high surface mass densities have a very narrow range of metallicities; however, at fixed mass, the spread in metallicity increases substantially with increasing galaxy size (decreasing density). We identify residual correlations with morphology and environment. At fixed mass and size, galaxies with late-type morphologies, small bulges and low Sérsic n are younger than early type, high n, high bulgeto- total galaxies. Both age and metallicity show small residual correlations with environment; at fixed mass and size, galaxies in denser environments or more massive haloes are older and somewhat more metal rich than those in less dense environments. We connect these trends to evolutionary tracks within the size-mass plane.

Original languageEnglish
Pages (from-to)2833-2855
Number of pages23
JournalMonthly Notices of the Royal Astronomical Society
Volume472
Issue number3
DOIs
Publication statusPublished - 2017 Jan 1

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galaxies
metallicity
stellar mass
metal
metals
spectrographs
halos
apertures
luminosity
trends
radii
augmentation

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Scott, Nicholas ; Brough, S. ; Croom, Scott M. ; Davies, Roger L. ; van de Sande, Jesse ; Allen, J. T. ; Bland-Hawthorn, Joss ; Bryant, Julia J. ; Cortese, Luca ; D'Eugenio, Francesco ; Federrath, Christoph ; Ferreras, Ignacio ; Goodwin, Michael ; Groves, Brent ; Konstantopoulos, Iraklis ; Lawrence, Jon S. ; Medling, Anne M. ; Moffett, Amanda J. ; Owers, Matt S. ; Richards, Samuel ; Robotham, A. S.G. ; Tonini, Chiara ; Yi, Sukyoung K. / The SAMI Galaxy Survey : Global stellar populations on the size-mass plane. In: Monthly Notices of the Royal Astronomical Society. 2017 ; Vol. 472, No. 3. pp. 2833-2855.
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abstract = "We present an analysis of the global stellar populations of galaxies in the SAMI (Sydney- AAO Multi-object Integral field spectrograph) Galaxy Survey. Our sample consists of 1319 galaxies spanning four orders of magnitude in stellar mass and includes all morphologies and environments. We derive luminosity-weighted, single stellar population equivalent stellar ages, metallicities and alpha enhancements from spectra integrated within one effective radius apertures. Variations in galaxy size explain the majority of the scatter in the age-mass and metallicity-mass relations. Stellar populations vary systematically in the plane of galaxy size and stellar mass, such that galaxies with high stellar surface mass density are older, more metal rich and alpha enhanced than less dense galaxies. Galaxies with high surface mass densities have a very narrow range of metallicities; however, at fixed mass, the spread in metallicity increases substantially with increasing galaxy size (decreasing density). We identify residual correlations with morphology and environment. At fixed mass and size, galaxies with late-type morphologies, small bulges and low S{\'e}rsic n are younger than early type, high n, high bulgeto- total galaxies. Both age and metallicity show small residual correlations with environment; at fixed mass and size, galaxies in denser environments or more massive haloes are older and somewhat more metal rich than those in less dense environments. We connect these trends to evolutionary tracks within the size-mass plane.",
author = "Nicholas Scott and S. Brough and Croom, {Scott M.} and Davies, {Roger L.} and {van de Sande}, Jesse and Allen, {J. T.} and Joss Bland-Hawthorn and Bryant, {Julia J.} and Luca Cortese and Francesco D'Eugenio and Christoph Federrath and Ignacio Ferreras and Michael Goodwin and Brent Groves and Iraklis Konstantopoulos and Lawrence, {Jon S.} and Medling, {Anne M.} and Moffett, {Amanda J.} and Owers, {Matt S.} and Samuel Richards and Robotham, {A. S.G.} and Chiara Tonini and Yi, {Sukyoung K.}",
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Scott, N, Brough, S, Croom, SM, Davies, RL, van de Sande, J, Allen, JT, Bland-Hawthorn, J, Bryant, JJ, Cortese, L, D'Eugenio, F, Federrath, C, Ferreras, I, Goodwin, M, Groves, B, Konstantopoulos, I, Lawrence, JS, Medling, AM, Moffett, AJ, Owers, MS, Richards, S, Robotham, ASG, Tonini, C & Yi, SK 2017, 'The SAMI Galaxy Survey: Global stellar populations on the size-mass plane', Monthly Notices of the Royal Astronomical Society, vol. 472, no. 3, pp. 2833-2855. https://doi.org/10.1093/MNRAS/STX2166

The SAMI Galaxy Survey : Global stellar populations on the size-mass plane. / Scott, Nicholas; Brough, S.; Croom, Scott M.; Davies, Roger L.; van de Sande, Jesse; Allen, J. T.; Bland-Hawthorn, Joss; Bryant, Julia J.; Cortese, Luca; D'Eugenio, Francesco; Federrath, Christoph; Ferreras, Ignacio; Goodwin, Michael; Groves, Brent; Konstantopoulos, Iraklis; Lawrence, Jon S.; Medling, Anne M.; Moffett, Amanda J.; Owers, Matt S.; Richards, Samuel; Robotham, A. S.G.; Tonini, Chiara; Yi, Sukyoung K.

In: Monthly Notices of the Royal Astronomical Society, Vol. 472, No. 3, 01.01.2017, p. 2833-2855.

Research output: Contribution to journalArticle

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AU - D'Eugenio, Francesco

AU - Federrath, Christoph

AU - Ferreras, Ignacio

AU - Goodwin, Michael

AU - Groves, Brent

AU - Konstantopoulos, Iraklis

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AU - Owers, Matt S.

AU - Richards, Samuel

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N2 - We present an analysis of the global stellar populations of galaxies in the SAMI (Sydney- AAO Multi-object Integral field spectrograph) Galaxy Survey. Our sample consists of 1319 galaxies spanning four orders of magnitude in stellar mass and includes all morphologies and environments. We derive luminosity-weighted, single stellar population equivalent stellar ages, metallicities and alpha enhancements from spectra integrated within one effective radius apertures. Variations in galaxy size explain the majority of the scatter in the age-mass and metallicity-mass relations. Stellar populations vary systematically in the plane of galaxy size and stellar mass, such that galaxies with high stellar surface mass density are older, more metal rich and alpha enhanced than less dense galaxies. Galaxies with high surface mass densities have a very narrow range of metallicities; however, at fixed mass, the spread in metallicity increases substantially with increasing galaxy size (decreasing density). We identify residual correlations with morphology and environment. At fixed mass and size, galaxies with late-type morphologies, small bulges and low Sérsic n are younger than early type, high n, high bulgeto- total galaxies. Both age and metallicity show small residual correlations with environment; at fixed mass and size, galaxies in denser environments or more massive haloes are older and somewhat more metal rich than those in less dense environments. We connect these trends to evolutionary tracks within the size-mass plane.

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