Bibcode
Serra, P.; McDermid, R. M.; Alatalo, K.; Blitz, L.; Bois, M.; Bournaud, F.; Bureau, M.; Cappellari, M.; Davies, R. L.; Davis, T. A.; de Zeeuw, P. T.; Emsellem, E.; Falcón-Barroso, J.; Khochfar, S.; Krajnović, D.; Kuntschner, H.; Lablanche, P.-Y.; Morganti, R.; Naab, T.; Sarzi, M.; Scott, N.; van den Bosch, R. C. E.; van de Ven, G.; Weijmans, A.; Young, L. M.
Bibliographical reference
PROBING STELLAR POPULATIONS OUT TO THE DISTANT UNIVERSE: CEFALU 2008, Proceedings of the International Conference. AIP Conference Proceedings, Volume 1111, pp. 111-114 (2009).
Advertised on:
5
2009
Citations
6
Refereed citations
5
Description
ATLAS3D is a multi-wavelength, volume-limited survey of 263
morphologically-selected early-type galaxies within a distance of 42 Mpc
and complete to MK<=-21.5. Here we present the ATLAS3D
project and our first results on the stellar populations of galaxies in
the ATLAS3D sample based on SAURON integral-field
spectroscopy. We show relations between integrated line-strength indices
and stellar velocity dispersion σ in the range
55<=σ(km/s)<=350. We derive
simple-stellar-population-equivalent age, metallicity and α/Fe
abundance ratio and discuss their relation to stellar velocity
dispersion, environment and galaxy internal kinematics. These
preliminary results indicate that slow rotators tend to be older and
have less variation in age than fast rotators. We also find that
galaxies in lower density environments are on average younger than those
in denser environments, as found by other authors.