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A&A 410, 803-812 (2003)
DOI: 10.1051/0004-6361:20031261
Stellar population gradient in lenticular galaxies: NGC 1023, NGC 3115 and NGC 4203
M. Bassin and Ch. BonattoUniversidade Federal do Rio Grande do Sul, Instituto de Física, CP 15051, Porto Alegre CEP 91501-970, RS, Brazil
(Received 11 March 2003 / Accepted 2 July 2003)
Abstract
We investigate the stellar population content in the lenticular galaxies
NGC 1023, NGC 3115 and NGC 4203 applying a population synthesis method based
on a seven component spectral basis with different ages -
,
,
,
,
,
and older than
1010 years, and metallicity in the range
.
This study employs two-dimensional STIS spectra in the range
2900-5700 Å,
obtained from the Hubble Space Telescope public archives. We extracted
one-dimensional spectra in adjacent windows 100 pc wide (projected distance)
from the nuclear regions up to 300-400 pc. The largest contribution, both in
5870 Å
flux and mass fraction, comes from old stars (age
>1010 years). We verified the
possible existence of circumnuclear bursts (CNBs) in NGC 3115 and NGC 4203.
Key words: galaxies: elliptical and lenticular, cD -- galaxies: stellar content -- galaxies: nuclei
Offprint request: Ch. Bonatto, charles@if.ufrgs.br
SIMBAD Objects
© ESO 2003
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