SIMBAD references

2008A&A...483...57S - Astronomy and Astrophysics, volume 483, 57-69 (2008/5-3)

Stellar populations, neutral hydrogen, and ionised gas in field early-type galaxies.

SERRA P., TRAGER S.C., OOSTERLOO T.A. and MORGANTI R.

Abstract (from CDS):

We present a study of the stellar populations of a sample of 39 local, field early-type galaxies whose HI properties are known from interferometric data. Our aim is to understand whether stellar age and chemical composition depend on the HI content of galaxies. We also study their ionised gas content and how it relates to the neutral hydrogen gas. Stellar populations and ionised gas are studied from optical long-slit spectra. We determine stellar age, metallicity and alpha-to-iron ratio by analysing a set of Lick/IDS line-strength indices measured from the spectra after modelling and subtracting the ionised-gas emission. We do not find any trend in the stellar populations parameters with M(HI). However, we do find that, at stellar velocity dispersion σ≤230km/s, 2/3 of the galaxies with less than 108M of HI are centrally rejuvenated, while none of the HI-richer systems is. Furthermore, none of the more massive, σ≥230 km/s -objects is centrally rejuvenated independently of their HI mass. Concerning the ionised gas, we detect emission in 60% of the sample. This is generally extended and always characterised by LINER-like emission-line ratios at any radius. We find that a large HI mass is necessary (but not sufficient) for a galaxy to host bright ionised-gas emission. A plausible interpretation of our results is that gas-rich mergers play a significant role in E/S0 formation, especially at lower σ. Within this picture, HI-poor, centrally-rejuvenated objects could form in mergers where gas angular-momentum removal (and therefore inflow) is efficient; HI-rich galaxies with no significant age gradients (but possibly uniformly young) could be formed in interactions characterised by high-angular momentum gas.

Abstract Copyright:

Journal keyword(s): galaxies: elliptical and lenticular, cD - galaxies: evolution - galaxies: interactions - galaxies: stellar content - galaxies: ISM

Simbad objects: 86

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2008A&A...483...57S and select 'bookmark this link' or equivalent in the popup menu


2019.12.13-14:04:06

© Université de Strasbourg/CNRS

    • Contact