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Stellar Populations of Elliptical Galaxies in Virgo Cluster. I. The Data and Stellar Population Analysis
Author(s) -
Y. Yamada,
N. Arimoto,
A. Vazdekis,
R. F. Peletier
Publication year - 2006
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/498252
Subject(s) - virgo cluster , astrophysics , physics , stellar population , elliptical galaxy , galaxy , metallicity , astronomy , data reduction , population , star formation , statistics , demography , mathematics , sociology
We have determined spectroscopic ages of elliptical galaxies in the Virgocluster using spectra of very high signal-to-noise ratio (S/N/A > 100). Weobserved 8 galaxies with the Subaru Telescope and have combined this samplewith 6 galaxies previously observed with the WHT. To determine their ages wehave used a new method based on the Hgamma_sigma age indicator, which isvirtually independent of the effects of metallicity. Apart from ages we haveestimated abundances of various elements. In this paper we present theobservations, the data reduction and the reliability of the Hgamma_sigmamethod. The results of this investigation are presented in a companion paper(Yamada et al. 2006).Comment: 33 pages, 9 figures, ApJ accepte

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