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相关论文: On the Radial Stellar Content of Early-Type Galaxi…

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We analyze the evolution of colour gradients predicted by the hydrodynamical models of early type galaxies (ETGs) in Pipino et al. (2008), which reproduce fairly well the chemical abundance pattern and the metallicity gradients of local…

宇宙学与河外天体物理 · 物理学 2015-06-16 C. Tortora , A. Pipino , A. D'Ercole , N. R. Napolitano , F. Matteucci

The most massive early-type galaxies (ETGs) are known to form through numerous galaxy mergers. Thus, it is intriguing to study whether their formation in low-density environments, where nearby companions are almost absent, is associated…

星系天体物理 · 物理学 2024-10-24 Yongmin Yoon , Jae-Woo Kim , Jongwan Ko

A detailed analysis of how environment affects the star formation history of early-type galaxies (ETGs) is undertaken via high signal to noise ratio stacked spectra obtained from a sample of 20,977 ETGs (morphologically selected) from the…

星系天体物理 · 物理学 2015-06-22 F. La Barbera , A. Pasquali , I. Ferreras , A. Gallazzi , R. R. de Carvalho , I. G. de la Rosa

The stellar mass-to-light ratio gradient in SDSS $r-$band $\nabla (M_*/L_r)$ of a galaxy depends on its mass assembly history, which is imprinted in its morphology and gradients of age, metallicity, and stellar initial mass function (IMF).…

星系天体物理 · 物理学 2021-08-25 Junqiang Ge , Shude Mao , Youjun Lu , Michele Cappellari , Richard J. Long , Renbin Yan

We report on a uniform comparative analysis of the fundamental parameters of early-type galaxies at z~1 down to a well defined magnitude limit (M_B\leq -20.0 in the field and M_B\leq -20.5 in the clusters). The changes in the M/L_B ratio…

天体物理学 · 物理学 2011-02-11 Sperello di Serego Alighieri , Barbara Lanzoni , Inger Jorgensen

We derive central values and logarithmic gradients for the Hbeta, Mg and Fe indices of 35 early-type galaxies in the Coma cluster. We find that pure elliptical galaxies have on average slightly higher velocity dispersions, lower Hbeta, and…

天体物理学 · 物理学 2008-11-26 D. Mehlert , D. Thomas , R. P. Saglia , R. Bender , G. Wegner

The environment is known to affect the formation and evolution of galaxies considerably best visible through the well-known morphology-density relationship. In this paper we study the effect of environment on the evolution of early-type…

宇宙学与河外天体物理 · 物理学 2015-05-14 Daniel Thomas , Claudia Maraston , Kevin Schawinski , Marc Sarzi , Joseph Silk

We derive stellar population parameters and radial gradients within 0.65 $R_e$ for spatially resolved spectra of 2968 early-type galaxies from MaNGA, spanning stellar velocity dispersions ($\sigma$) of 50--340 km s$^{-1}$. Light-weighted…

星系天体物理 · 物理学 2025-11-04 Tathagata Pal , Guy Worthey

We use a combination of deep optical and near-infrared light profiles for a morphologically diverse sample of Virgo cluster galaxies to study the radially-resolved stellar populations of cluster galaxies over a wide range of galaxy…

宇宙学与河外天体物理 · 物理学 2015-05-20 Joel C. Roediger , Stephane Courteau , Lauren A. MacArthur , Michael McDonald

Recent observations have revealed that early-type galaxies (ETG) in clusters comprise an old galaxy population that is evolving passively. We review some recent observations from the ground and from HST that show that ETG have undergone a…

This paper explores if the mean properties of Early-Type Galaxies (ETG) can be reconstructed from "genetic" information stored in their GCs (i.e., in their chemical abundances, spatial distributions and ages). This approach implies that the…

星系天体物理 · 物理学 2015-06-19 J. C. Forte , E. I. Vega , F. R. Faifer , A. V. Smith Castelli , Carlos Escudero , N. M. González , L. A. Sesto

A comparison is made between the age-metallicity relation obtained from four different types of studies: F and G stars in the Solar Neighbourhood, analysis of open clusters, galactic structure studies with the stellar population synthesis…

天体物理学 · 物理学 2009-10-30 G. Carraro , Y. K. Ng , L. Portinari

The stellar populations of galaxies hold vital clues to their formation histories. In this paper we present results based on modeling stacked spectra of early-type galaxies drawn from the Sloan Digital Sky Survey (SDSS) as a function of…

宇宙学与河外天体物理 · 物理学 2015-06-15 Charlie Conroy , Genevieve Graves , Pieter van Dokkum

A simple model of chemical enrichment in cluster early-type galaxies is presented where the main parameters driving the formation of the stellar component are reduced to four: infall timescale (tf), formation epoch (zF), star formation…

天体物理学 · 物理学 2009-10-31 I. Ferreras , J. Silk

The correlation between [Mg/Fe] and galaxy mass found in elliptical galaxies sets a strong constraint on the duration of star formation. Furthermore, the colour-magnitude relation restricts the range of ages and metallicities of the stellar…

天体物理学 · 物理学 2009-11-07 I. Ferreras , J. Silk

Early-type dwarf galaxies are not simply featureless, old objects, but were found to be much more diverse, hosting substructures and a variety of stellar population properties. To explore the stellar content of faint early-type galaxies,…

We present a study of internal stellar population gradients in early-type cluster galaxies. Using the VLT VIMOS integral field unit, we observed 19 galaxies in the core of the Shapley Supercluster (z = 0.048). The radial trends in nine…

宇宙学与河外天体物理 · 物理学 2015-05-14 T. D. Rawle , Russell J. Smith , J. R. Lucey

We present radial stellar population parameters for a subsample of 12 galaxies from the 36 isolated early-type galaxies of Reda et al. Using new long-slit spectra, central values and radial gradients for the stellar age, metallicity [Z/H]…

天体物理学 · 物理学 2008-11-26 Fatma M. Reda , Robert N. Proctor , Duncan A. Forbes , George K. T. Hau , Søren S. Larsen , ;

We measure the stellar populations as a function of radius for 90 early-type galaxies (ETGs) in the MASSIVE survey, a volume-limited integral-field spectroscopic (IFS) galaxy survey targeting all northern-sky ETGs with absolute K-band…