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相关论文: Nature and nurture of early-type dwarf galaxies in…

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We present the stellar population properties of 13 dwarf galaxies residing in poor groups (low-density environment, LDE) observed with VIMOS@VLT. Ages, metallicities, and [alpha/Fe] ratios were derived from the Lick indices Hbeta, Mgb,…

宇宙学与河外天体物理 · 物理学 2015-05-20 F. Annibali , R. Grutzbauch , R. Rampazzo , A. Bressan , W. W. Zeilinger

In this paper we study the underlying stellar population of a sample of 65 nearby early-type galaxies predominantly located in low density environments. Ages, metallicities and [alpha/Fe] ratios have been derived through the comparison of…

天体物理学 · 物理学 2010-10-28 F. Annibali , A. Bressan , R. Rampazzo , W. W. Zeilinger , L. Danese

We have investigated the properties of a volume and magnitude limited sample of nearby early type galaxies that were carefully selected from the AAO two degree field galaxy redshift survey. We used images from the DSS to confirm the E/S0…

天体物理学 · 物理学 2009-11-11 M. Collobert , M. Sarzi , R. L. Davies , H. Kuntschner , Matthew Colless

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

Dwarf galaxies are the numerically dominating population in the dense regions of the universe. Although they seem to be simple systems at first view, the stellar populations of dwarf elliptical galaxies (dEs) might be fairly complex.…

宇宙学与河外天体物理 · 物理学 2015-05-14 S. Paudel , T. Lisker

(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

Dwarf galaxies, as the most numerous type of galaxy, offer the potential to study galaxy formation and evolution in detail in the nearby Universe. Although they seem to be simple systems at first view, they remain poorly understood. In an…

We explore the environmental dependence of star formation timescales in low mass galaxies using the [$\alpha$/Fe] abundance ratio as an evolutionary clock. We present integrated [$\alpha$/Fe] measurements for 11 low mass ($M_\star \sim…

We present kinematics and stellar population properties of 17 dwarf early-type galaxies in the luminosity range -14> M_B> -19. Our sample fills the gap between the intensively studied giant elliptical and Local Group dwarf spheroidal…

天体物理学 · 物理学 2009-11-07 D. Thomas , R. Bender , U. Hopp , C. Maraston , L. Greggio

We investigate the interplay between morphology, specific star formation rate (sSFR), and local environment using a sample of 7,408 galaxies from the SDSS-IV MaNGA survey. Our analysis spans stellar masses from dwarf to massive galaxies,…

星系天体物理 · 物理学 2026-05-20 Chandan Watts , Gothai L , Sudhanshu Barway

We investigate in detail 13 early-type field galaxies with 0.2<z<0.7 drawn from the FORS Deep Field. Since the majority (9 galaxies) is at z~0.4, we compare the field galaxies to 22 members of three rich clusters with z=0.37 to explore…

天体物理学 · 物理学 2010-10-28 B. L. Ziegler , D. Thomas , A. Boehm , R. Bender , A. Fritz , C. Maraston

The aim of this paper is to set constraints of the epochs of early-type galaxy formation through the 'archaeology' of the stellar populations in local galaxies. Using our models of absorption line indices that account for variable abundance…

天体物理学 · 物理学 2009-07-09 D. Thomas , C. Maraston , R. Bender , C. Mendes de Oliveira

[Abridged] Using VLT/FORS2 spectroscopy, we have studied the properties of the central stellar populations of a sample of 38 nucleated early-type dwarf (dE) galaxies in the Virgo Cluster. We find that these galaxies do not exhibit the same…

宇宙学与河外天体物理 · 物理学 2015-05-18 S. Paudel , T. Lisker , H. Kuntschner , E. Grebel , K. Glatt

We have acquired intermediate resolution spectra in the 3700-7000 A wavelength range for a sample of 65 early-type galaxies predominantly located in low density environments, a large fraction of which show emission lines. The spectral…

天体物理学 · 物理学 2007-05-23 F. Annibali , A. Bressan , R. Rampazzo , W. Zeilinger , L. Danese

We analyse the Fundamental Plane (FP) relation of $39,993$ early-type galaxies (ETGs) in the optical (griz) and $5,080$ ETGs in the Near-Infrared (YJHK) wavebands, forming an optical$+$NIR sample of $4,589$ galaxies. We focus on the…

宇宙学与河外天体物理 · 物理学 2015-05-18 F. La Barbera , P. A. A. Lopes , R. R. de Carvalho , I. G. de la Rosa , A. A. Berlind

Using MUSE data, we investigate the radial gradients of stellar population properties (namely age, [M/H], and the abundance ratio of $\alpha$ elements [$\alpha$/Fe]) for a sample of nine dwarf early-type (dE) galaxies with…

We compute new population synthesis models of Lick absorption line indices with variable alpha/Fe ratios and use them to derive average ages, metallicities, and alpha/Fe element enhancements for a sample of 126 field and cluster early-type…

天体物理学 · 物理学 2007-05-23 Daniel Thomas , Claudia Maraston , Ralf Bender

We define a volume limited sample of over 14,000 early-type galaxies (ETGs) selected from data release six of the Sloan Digital Sky Survey. The density of environment of each galaxy is robustly measured. By comparing narrow band spectral…

天体物理学 · 物理学 2009-11-13 M. S. Clemens , A. Bressan , B. Nikolic , R. Rampazzo

We use a complete sample of 211 nearby (z<0.08) dwarf (10^8 MSun < Mstar < 10^9.5 Msun) galaxies in low-density environments, to study their structural properties: effective radii (R_e), effective surface brightnesses (mu_e) and colour…

星系天体物理 · 物理学 2024-09-05 Ilin Lazar , Sugata Kaviraj , Aaron E. Watkins , Garreth Martin , Brian Bichang'a , Ryan A. Jackson

We present the photometric properties of 2210 newly identified dwarf galaxy candidates in the MATLAS fields. The Mass Assembly of early Type gaLAxies with their fine Structures (MATLAS) deep imaging survey mapped $\sim$142 deg$^2$ of the…

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