Issue |
A&A
Volume 429, Number 2, January II 2005
|
|
---|---|---|
Page(s) | 477 - 487 | |
Section | Extragalactic astronomy | |
DOI | https://doi.org/10.1051/0004-6361:20041591 | |
Published online | 17 December 2004 |
Abundances and kinematics of a candidate sub-damped Lymanα galaxy toward PHL 1226*
1
Astrophysikalisches Institut Potsdam, An der Sternwarte 16, 14482 Potsdam, Germany e-mail: lchristensen@aip.de
2
Department of Physics & Astronomy, University of Pittsburgh, 3941 O'Hara Street, Pittsburgh, PA 15260, USA
3
Institut für Physik, Universität Potsdam, Am Neuen Palais 10, 14469 Potsdam, Germany
Received:
3
July
2004
Accepted:
8
September
2004
The spectrum of the quasar PHL 1226 is known to have a
strong and sub-damped Lymanα (sub-DLA) absorption line
system with
cm-2 at
.
Using integral field spectra from the Potsdam Multi Aperture
Spectrophotometer (PMAS) we investigate a galaxy at an impact parameter of
6
4 which is most probably responsible for the absorption lines. A
fainter galaxy at a similar redshift and a slightly larger distance from the
QSO is known to exist, but we assume that the absorption is caused by the
more nearby galaxy. From optical Balmer lines we estimate an intrinsic
reddening consistent with 0, and a moderate star formation rate of
0.5 M
is inferred from the Hα luminosity. Using
nebular emission line ratios we find a solar oxygen abundance
and a solar nitrogen to oxygen abundance
ratio
. This abundance is larger than those
of all known sub-DLA systems derived from analyses of metal absorption lines
in quasar spectra. On the other hand, the properties are compatible with the
most metal rich galaxies responsible for strong
absorption
systems. These two categories can be reconciled if we assume an abundance
gradient similar to local galaxies. Under that assumption we predict
abundances
and
for the
sub-DLA cloud, which is similar to high redshift DLA and sub-DLA systems.
We find evidence for a rotational velocity of ~200 km s-1 over a
length of ~7 kpc. From the geometry and kinematics of the galaxy we
estimate that the absorbing cloud does not belong to a rotating disk, but
could originate in a rotating halo.
Key words: galaxies: abundances / galaxies: kinematics and dynamics / quasars: individual: PHL 1226
© ESO, 2005
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