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26 April 2024
 
  » arxiv » astro-ph/0508520

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Nearby early-type galaxies with ionized gas.II. Line-strength indices for 18 additional galaxies
F. Annibali ; A. Bressan ; R. Rampazzo ; W. W. Zeilinger ;
Date 24 Aug 2005
Subject astro-ph
Affiliation1, 2), R. Rampazzo , W. W. Zeilinger ( SISSA INAF, Osservatorio Astronomico di Padova Inst. fur Astronomie der Universitat Wien
AbstractRampazzo et al. 2005 (Paper I) presented a data-set of line-strength indices for 50 early-type galaxies in the nearby Universe. The galaxy sample is biased toward galaxies showing emission lines, located in environments corresponding to a broad range of local galaxy densities, although predominantly in low density environments. The present addendum to Paper I enlarges the above data-set of line-strength indices by analyzing 18 additional early-type galaxies (three galaxies, namely NGC 3607, NGC 5077 and NGC 5898 have been already presented in the previous set). As in Paper I, we measured 25 line-strength indices, defined by the Lick IDS "standard" system (Trager et al. 1998; Worthey & Ottaviani 1997), for 7 luminosity weighted apertures and 4 gradients of each galaxy. This paper presents the line-strength data-set and compares it with the available data in the literature.
Source arXiv, astro-ph/0508520
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