TY - JOUR

T1 - Insights into formation scenarios of massive early-type galaxies from spatially resolved stellar population analysis in CALIFA

AU - Zibetti, Stefano

AU - Gallazzi, Anna R.

AU - Hirschmann, Michaela

AU - Consolandi, Guido

AU - Falcon-Barroso, Jesus

AU - van de Ven, Glenn

AU - Lyubenova, Mariya

PY - 2020/1/2

Y1 - 2020/1/2

N2 - We perform spatially resolved stellar population analysis for a sample of 69 early-type galaxies (ETGs) from the CALIFA integral field spectroscopic survey, including 48 ellipticals and 21 S0's. We generate and quantitatively characterize profiles of light-weighted mean stellar age and metallicity within less than or similar to 2R(e), as a function of radius and stellar-mass surface density mu(*). We study in detail the dependence of profiles on galaxies' global properties, including velocity dispersion se, stellarmass, morphology. ETGs are universally characterized by strong, negative metallicity gradients (similar to-0.3 dex per R-e) within 1R(e), which flatten out moving towards larger radii. A quasi-universal local mu(*)-metallicity relation emerges, which displays a residual systematic dependence on se, whereby higher se implies higher metallicity at fixed mu(*). Age profiles are typically U-shaped, with minimum around 0.4 R-e, asymptotic increase to maximum ages beyond similar to 1.5 R-e, and an increase towards the centre. The depth of the minimum and the central increase anticorrelate with sigma(e). A possible qualitative interpretation of these observations is a two-phase scenario. In the first phase, dissipative collapse occurs in the inner 1R(e), establishing a negative metallicity gradient. The competition between the outside-in quenching due to feedback-driven winds and some form of inside-out quenching, possibly caused by central AGN feedback or dynamical heating, determines the U-shaped age profiles. In the second phase, the accretion of ex-situ stars from quenched and low-metallicity satellites shapes the flatter stellar population profiles in the outer regions.

AB - We perform spatially resolved stellar population analysis for a sample of 69 early-type galaxies (ETGs) from the CALIFA integral field spectroscopic survey, including 48 ellipticals and 21 S0's. We generate and quantitatively characterize profiles of light-weighted mean stellar age and metallicity within less than or similar to 2R(e), as a function of radius and stellar-mass surface density mu(*). We study in detail the dependence of profiles on galaxies' global properties, including velocity dispersion se, stellarmass, morphology. ETGs are universally characterized by strong, negative metallicity gradients (similar to-0.3 dex per R-e) within 1R(e), which flatten out moving towards larger radii. A quasi-universal local mu(*)-metallicity relation emerges, which displays a residual systematic dependence on se, whereby higher se implies higher metallicity at fixed mu(*). Age profiles are typically U-shaped, with minimum around 0.4 R-e, asymptotic increase to maximum ages beyond similar to 1.5 R-e, and an increase towards the centre. The depth of the minimum and the central increase anticorrelate with sigma(e). A possible qualitative interpretation of these observations is a two-phase scenario. In the first phase, dissipative collapse occurs in the inner 1R(e), establishing a negative metallicity gradient. The competition between the outside-in quenching due to feedback-driven winds and some form of inside-out quenching, possibly caused by central AGN feedback or dynamical heating, determines the U-shaped age profiles. In the second phase, the accretion of ex-situ stars from quenched and low-metallicity satellites shapes the flatter stellar population profiles in the outer regions.

KW - techniques: imaging spectroscopy

KW - galaxies: abundances

KW - galaxies: elliptical and lenticular, cD

KW - galaxies: evolution

KW - galaxies:formation

KW - galaxies: stellar content

KW - POTSDAM MULTIAPERTURE SPECTROPHOTOMETER

KW - STAR-FORMATION HISTORIES

KW - SAURON PROJECT

KW - METALLICITY GRADIENTS

KW - ATLAS(3D) PROJECT

KW - SIMPLE-MODEL

KW - CLUSTER

KW - AGES

KW - SPECTROSCOPY

KW - ABSORPTION

U2 - 10.1093/mnras/stz3205

DO - 10.1093/mnras/stz3205

M3 - Journal article

VL - 491

SP - 3562

EP - 3585

JO - Royal Astronomical Society. Monthly Notices

JF - Royal Astronomical Society. Monthly Notices

SN - 0035-8711

IS - 3

ER -