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Chandra Observations of the Stellar Populations and Diffuse Gas in Nearby Galaxies

A. Zezas·G. Fabbiano·A. Prestwich·M. Ward·S. Murray
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Abstract

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.

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A. Zezas, G. Fabbiano, A. Prestwich, M. Ward, S. Murray. 2001-09-19. Chandra Observations of the Stellar Populations and Diffuse Gas in Nearby Galaxies. https://arxiv.org/abs/astro-ph/0109302

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