-
Articles citing this article
-
Same authors
- Recommend this article
- Download citation
- Alert me if this article is cited
- Alert me if this article is corrected
|
||||||||||||||||||
A&A 431, 127-142 (2005)
DOI: 10.1051/0004-6361:20047042
Thick disks and halos of spiral galaxies M 81, NGC 55 and NGC 300
N. A. Tikhonov1, 2, O. A. Galazutdinova1, 2 and I. O. Drozdovsky3, 41 Special Astrophysical Observatory, Russian Academy of Sciences, N. Arkhyz, KChR 369167, Russia
e-mail: ntik@sao.ru
2 Isaac Newton Institute of Chile, SAO Branch, Russia
3 Spitzer Science Center, Caltech, MC 220-6, Pasadena, CA 91125, USA
4 Astronomical Institute, St. Petersburg University, 198504, Russia
(Received 9 January 2004 / Accepted 28 September 2004)
Abstract
By using images from the HST/WFPC2/ACS archive, we have analyzed the
spatial distribution of the AGB and RGB stars along the galactocentric radius
of nearby spiral galaxies M 81, NGC 300 and NGC 55.
Examining color-magnitude diagrams and stellar luminosity functions, we gauge
the stellar contents of the surroundings of the three galaxies.
The red giant population (RGB) identified at large galactocentric radii yields
a distance of
Mpc for M 81,
Mpc for NGC 55,
and
Mpc for NGC 300, and a mean stellar metallicity of
-0.65,
-1.25, and
-0.87 respectively. We find that there are two number density gradients
of RGB stars along the radius, which correspond to the thick disk and halo
components of the galaxies. We confirm the presence of a metallicity gradient
of evolved stars in these galaxies, based on the systematic changes of the
color distribution of red giant stars.
These results imply that the thick disk might be a general feature of
spiral galaxies, and endorse a further investigation of the outer stellar
edges of nearby spirals, which is critical in constraining the origin
and evolution of galaxies.
Key words: galaxies: individual: M 81 -- galaxies: individual: NGC 55 -- galaxies: individual: NGC 300 -- galaxies: stellar content -- galaxies: photometry -- galaxies: structure
SIMBAD Objects
© ESO 2005
| What is OpenURL? |
- If your librarian has set up your subscription with an OpenURL resolver, OpenURL links appear automatically on the abstract pages.
- You can define your own OpenURL resolver with your EDPS Account. In this case your choice will be given priority over that of your library.
- You can use an add-on for your browser (Firefox or I.E.) to display OpenURL links on a page (see http://www.openly.com/openurlref/). You should disable this module if you wish to use the OpenURL server that you or your library have defined.

BibSonomy
CiteUlike
Connotea
Del.icio.us
Digg
Facebook