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相关论文: Stellar Populations in Nearby Lenticular Galaxies

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The properties of stellar populations in the centers of 54 nearby lenticular galaxies are investigated by means of 2D spectroscopy, with the Multi-Pupil Spectrograph of the 6m telescope of SAO RAS; the unresolved nuclei and their…

天体物理学 · 物理学 2009-11-10 Olga K. Silchenko

Panoramic spectroscopic data of the sample of 80 nearby lenticular galaxies obtained with the Multi-Pupil Fiber Spectrograph of the 6-m telescope are presented. The SSP-equivalent ages, [Z/H], and [Mg/Fe] are determined through the Lick…

天体物理学 · 物理学 2009-11-13 Olga K. Sil'chenko

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

Spectral line indices for a sample of 290 nearby E and S0 galaxies are used to investigate the stellar populations of these galaxies. Relations are established between the line indices (Mg2, <Fe>, Hbeta) and the velocity dispersions, the…

天体物理学 · 物理学 2015-06-24 Inger Jorgensen

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

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 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

By undertaking deep long-slit spectroscopy with the focal reducer SCORPIO of the Russian 6m telescope, we studied stellar population properties and their variation with radius in 15 nearby S0 galaxies sampling a wide range of luminosities…

宇宙学与河外天体物理 · 物理学 2023-02-01 O. K. Sil'chenko , I. S. Proshina , A. P. Shulga , S. E. Koposov

Photometry and long-slit spectroscopy are presented for 14 S0 and spiral galaxies of the Fornax, Eridanus and Pegasus cluster, and NGC 7582 group. The structural parameters of the galaxies are derived from the R-band images by performing a…

天体物理学 · 物理学 2009-11-13 L. Morelli , E. Pompei , A. Pizzella , J. Méndez-Abreu , E. M. Corsini , L. Coccato , R. P. Saglia , M. Sarzi , F. Bertola

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

In this paper we present the results of long-slit spectral observations for a sample of isolated lenticular galaxies, made with the SCORPIO and SCORPIO-2 spectrographs of the 6-meter BTA telescope of the SAO RAS. By applying full spectral…

星系天体物理 · 物理学 2015-06-22 Ivan Katkov , Olga Sil'chenko , Victor Afanasiev

We present line-strengths and kinematics from the central regions of 32 galaxies with Hubble types ranging from E to Sbc. Spectral indices, based on the Lick system, are measured in the optical and near infra-red (NIR). The 24 indices…

天体物理学 · 物理学 2008-11-26 R. N. Proctor , A. E. Sansom

This paper is part of a series devoted to the study of the stellar populations in brightest cluster galaxies (BCGs), aimed at setting constraints on the formation and evolution of these objects. We have obtained high signal-to-noise ratio,…

宇宙学与河外天体物理 · 物理学 2015-05-13 S. I. Loubser , P. Sanchez-Blazquez , A. E. Sansom , I. K. Soechting

(Abridged) We study the nuclear star clusters in spiral galaxies of various Hubble types using spectra obtained with STIS on-board HST. We observed the nuclear clusters in 40 galaxies, selected from two previous HST/WFPC2 imaging surveys.…

We present photometry and long-slit spectroscopy for 12 S0 and spiral galaxies selected from the Catalogue of Isolated Galaxies. The structural parameters of the sample galaxies are derived from the Sloan Digital Sky Survey i-band images by…

星系天体物理 · 物理学 2016-10-05 L. Morelli , M. Parmiggiani , E. M. Corsini , L. Costantin , E. Dalla Bontà , J. Mèndez-Abreu , A. Pizzella

The influence of environment on the formation and evolution of early-type galaxies is, as yet, an unresolved issue. Constraints can be placed on models of early-type galaxy formation and evolution by examining their stellar populations as a…

宇宙学与河外天体物理 · 物理学 2015-05-19 Craig Harrison , Matthew Colless , Harald Kuntschner , Warrick Couch , Roberto De Propris , Michael Pracy

We report preliminary results of the characterization of bulge and inner disk stellar populations for 8 nearby spiral galaxies using Gemini/GMOS. The long-slit spectra extend out to 1-2 disk scale lengths with S/N/Ang > 50. Two different…

天体物理学 · 物理学 2009-11-13 Lauren A. MacArthur , Jesus Gonzalez , Stephane Courteau

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

We use detailed modeling of stellar populations of nearby galaxies to calculate population parameters. Our sample of galaxies includes most galaxies of the Local Group and several more distant giant galaxies. Available data are sufficient…

天体物理学 · 物理学 2007-05-23 J. Einasto , P. Tenjes

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
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