Astronomy and Astrophysics – Astrophysics
Scientific paper
2001-09-19
Astronomy and Astrophysics
Astrophysics
6 pages, 6 figures, To appear in the proceedings of the conference "The Central kpc of Starburst and AGN", APS Conference Seri
Scientific paper
We present Chandra observations of two star-forming galaxies (M82 and the Antennae) and three starburst/AGN composite galaxies (NGC1808, NGC6240, NGC7331). In both star-forming galaxies we detect a large number of sources with diverse properties. Some of them can be identified as X-ray binaries, based on their variability and spectra. However, there is a significant number of very soft and/or extended sources which could be supernova remnants. These observations confirm previous indications that there is a population of sources with X-ray luminosities much higher than the Eddington limit for a neutron star, suggesting that these objects are abundant in star-forming galaxies. We find the the X-ray luminosity functions of the discrete sources in these two galaxies are very similar. In the case of the composite galaxies we find that the AGN does not dominate their X-ray emission. A significant fraction of the emission from these objects is extended but there are also X-ray sources associated with circumnuclear star-formation.
Fabbiano Giuseppina
Murray Stephen S.
Prestwich Andrea
Ward Martin
Zezas Andreas
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