Issue |
A&A
Volume 449, Number 2, April II 2006
|
|
---|---|---|
Page(s) | 519 - 532 | |
Section | Extragalactic astronomy | |
DOI | https://doi.org/10.1051/0004-6361:20053923 | |
Published online | 21 March 2006 |
Peculiarities and populations in elliptical galaxies
III. Dating the last star formation event
Observatoire de Paris, LERMA, 77 Av. Denfert-Rochereau, 75015 Paris, France e-mail: raymond.michard@obspm.fr
Received:
26
July
2005
Accepted:
17
November
2005
Using 6 colours and 4 Lick line-indices we derive two-component models of
the populations of ellipticals, involving a “primary” and a “juvenile” population.
The first component is defined by the regressions of indices
against the central velocity dispersion found in Papers I and II for the sample
of non-peculiar objects. The second one is approximated by an
SSP, and the modeling derives its age A, metallicity Z and fractional V-luminosity
qV, the fractional mass qM being found therefrom. The model is designed for
“blueish” peculiar galaxies, i.e. the
sample and NGC 2865 family in the
terminology of Paper I. The morphological peculiarities and the population anomaly
are then believed to involve the same event, i.e. a merger plus starburst.
It is possible to improve the models in a few cases
by introducing diffuse dust (as suggested by far IR data), and/or by taking into
account the fact that Lick- and colour indices do not relate to identical galaxy
volumes. In most of the cases, the mass ratio of young stars qM seems too small
for the product of a recent major merger: the events under consideration might be
minor mergers bringing “the final touch” to the build-up of the structure
of the E-type object.
The same modeling has been successfully applied to blueish galaxies of
the
sample, without morphological peculiarities however, to support
the occurence of a distinct perturbing event.
A few reddish objects of the
sample (NGC 3923 family) and of the
sample are also modeled, in terms of an excess of high metallicity stars, or diffuse
dust, or both, but the results are inconclusive.
Key words: galaxies: elliptical and lenticulars, CD
© ESO, 2006
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