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相关论文: Stellar population gradients in early-type cluster…

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We present results from a pilot study of radial stellar population trends in early-type galaxies using the VLT VIMOS integral field unit (IFU). We observe twelve galaxies in the cluster Abell 3389 (z~0.027). For each galaxy, we measure 22…

天体物理学 · 物理学 2009-11-13 T. D. Rawle , Russell J. Smith , J. R. Lucey , A. M. Swinbank

We use high signal-to-noise spectroscopy for a sample of 232 quiescent galaxies in the Shapley Supercluster, to investigate how their stellar populations depend on velocity dispersion, luminosity and stellar mass. The sample spans a large…

宇宙学与河外天体物理 · 物理学 2015-05-14 Russell J. Smith , John R. Lucey , Michael J. Hudson

We present the results of a study of stellar population properties at large galactocentric radii of 14 low-mass early-type galaxies in the Fornax and Virgo clusters. We derive radial profiles of Age, total metallicity [Z/H], and [alpha/Fe]…

宇宙学与河外天体物理 · 物理学 2015-05-19 Max Spolaor , Chiaki Kobayashi , Duncan A. Forbes , Warrick J. Couch , George K. T. Hau

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 , ;

The evolution of galaxies is imprinted in their stellar populations. Several stellar population properties in massive early-type galaxies have been shown to correlate with intrinsic galaxy properties like the galaxy's central velocity…

星系天体物理 · 物理学 2021-12-22 A. Feldmeier-Krause , I. Lonoce , W. L. Freedman

We present line-strength gradients for 22 spectral indices measured in a sample of 82 early-type galaxies in different environments,including the high-density core of the Coma cluster, the Virgo cluster,poor groups,and field galaxies. We…

天体物理学 · 物理学 2009-11-11 P. Sanchez-Blazquez , J. Gorgas , N. Cardiel

The degree of influence that environment and mass have on the stellar populations of early-type galaxies is uncertain. In this paper we present the results of a spectroscopic analysis of the stellar populations of early-type galaxies aimed…

宇宙学与河外天体物理 · 物理学 2015-05-20 Craig Harrison , Matthew Colless , Harald Kuntschner , Warrick Couch , Roberto De Propris , Michael Pracy

(Abridged) We present a comprehensive analysis of the spatially resolved stellar population properties of 26 early-type dwarf (dE) galaxies in the Virgo cluster. Using Lick/IDS absorption line indices we derive simple stellar…

星系天体物理 · 物理学 2015-05-20 Sanjaya Paudel , Thorsten Lisker , Harald Kuntschner

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

We present the stellar population and velocity dispersion gradients for a sample of 24 brightest cluster galaxies (BCGs) in the nearby Universe for which we have obtained high quality long-slit spectra at the Gemini telescopes. With the aim…

宇宙学与河外天体物理 · 物理学 2015-06-04 S. I. Loubser , P. Sanchez-Blazquez

We present new optical spectroscopy for 342 R<18 galaxies in the Shapley Supercluster obtained with the AAOmega facility at the Anglo-Australian Telescope. We describe the observations and measurements of central velocity dispersion,…

天体物理学 · 物理学 2009-11-13 Russell J. Smith , John R. Lucey , Michael J. Hudson

We present an unbiased method for evaluating the ranges of ages and metallicities which are allowed by the photometric properties of the stellar populations that dominate the light of early-type galaxies in clusters. The method is based on…

天体物理学 · 物理学 2009-10-30 I. Ferreras , S. Charlot , J. Silk

We study the internal radial gradients of the stellar populations in a sample comprising 522 early-type galaxies (ETGs) from the SAMI (Sydney- AAO Multi-object Integral field spectrograph) Galaxy Survey. We stack the spectra of individual…

We present the analysis of the radial gradients of stellar absorption lines in a sample of 32 bulges of edge-on spiral galaxies, spanning nearly the full Hubble sequence (from S0 to Sc types), and a large range of velocity dispersion (from…

天体物理学 · 物理学 2009-11-13 P. Jablonka , J. Gorgas , P. Goudfrooij

This is the second paper of a series devoted to study the stellar content of early-type galaxies. The goal of the series is to set constraints on the evolutionary status of these objects. We use a new set of models which include an improved…

天体物理学 · 物理学 2009-11-11 P. Sanchez-Blazquez , J. Gorgas , N. Cardiel , J. J. Gonzalez

We examine the stellar population radial gradients (age, metallicity and [$\alpha/$Fe]) of $\sim$ 100 passive central galaxies up to $\sim 2 R_e$. The targeted groups have a halo mass range spanning from $11 < \log(M_{200}/M_{\odot}) < 15$,…

We present a study of the inner (out to $\sim$1 R$_{\mathrm{eff}}$) stellar populations of 9 shell galaxies. We derive stellar population parameters from long slit spectra by both analyzing the Lick indices of the galaxies and by fitting…

星系天体物理 · 物理学 2017-10-11 S. Carlsten , G. K. T. Hau , A. Zenteno

We present a detailed spatial analysis of stellar populations based on long-slit optical spectra in a sample of eight luminous early-type galaxies selected from nearby sparse groups and pairs, three of them may be interacting with a galaxy…

星系天体物理 · 物理学 2018-06-11 D. A. Rosa , A. C. Milone , A. C. Krabbe , I. Rodrigues

We present stellar population age and metallicity trends for a sample of 59 S0 galaxies based on optical SDSS and NIR J & H photometry. When combined with optical g and r passband imaging data from the SDSS archive and stellar population…

宇宙学与河外天体物理 · 物理学 2015-05-20 L. C. Prochaska Chamberlain , Stephane Courteau , Michael McDonald , James A. Rose

We examine stellar population gradients in ~100 massive early type galaxies spanning 180 < sigma* < 370 km/s and M_K of -22.5 to -26.5 mag, observed as part of the MASSIVE survey (Ma et al. 2014). Using integral-field spectroscopy from the…

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