Volume 490, Number 1, October IV 2008
|Page(s)||37 - 43|
|Published online||01 July 2008|
Universal X-ray emissivity of the stellar population in early-type galaxies: unresolved X-ray sources in NGC 3379
Max-Planck-Institute für Astrophysik, Karl-Schwarzschild-Str. 1, 85740 Garching bei München, Germany e-mail: firstname.lastname@example.org
2 Space Research Institute, Russian Academy of Sciences, Profsoyuznaya 84/32, 117997 Moscow, Russia
3 Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA
Accepted: 25 June 2008
We use deep Chandra observations to measure the emissivity of the unresolved X-ray emission in the elliptical galaxy NGC 3379. After elimination of bright, low-mass X-ray binaries with luminosities 1036 erg s-1, we find that the remaining unresolved X-ray emission is characterized by an emissivity per unit stellar mass 1027 erg s-1 in the 0.5-2 keV energy band. This value is in good agreement with those previosuly determined for the dwarf elliptical galaxy M 32, the bulge of the spiral galaxy M 31 and the Milky Way, as well as with the integrated X-ray emissivity of cataclysmic variables and coronally active binaries in the Solar neighborhood. This strongly suggests that i) the bulk of the unresolved X-ray emission in NGC 3379 is produced by its old stellar population; and ii) the old stellar populations in all galaxies can be characterized by a universal value of X-ray emissivity per unit stellar mass or per unit K band luminosity.
Key words: galaxies: bulges / X-rays: binaries / X-rays: galaxies / X-rays: ISM / galaxies: fundamental parameters
© ESO, 2008
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