A publishing partnership

On the Contribution of Unresolved Galactic Stars to the Diffuse Soft X-Ray Background

and

© 2001. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation K. D. Kuntz and S. L. Snowden 2001 ApJ 554 684 DOI 10.1086/321421

0004-637X/554/2/684

Abstract

Using stellar luminosity functions derived from ROSAT data, the contributions of Galactic stars to the diffuse X-ray background are calculated for ROSAT PSPC energy bands. The model follows that of Guillout and coworkers but uses ROSAT rather than Einstein data to determine the intrinsic luminosity distributions. The model adequately predicts the numbers of stellar sources observed in deep ROSAT surveys. The contribution of unresolved stellar sources to the ROSAT All-Sky Survey at the Galactic poles is 6.85, 4.76, and 4.91 × 10-6 counts s-1 arcmin-2 in bands R12 ( keV), R45 ( keV), and R67 (1.5 keV), respectively, which is equivalent to 4.66, 31.3, and 26.9 × 10-14 ergs cm-2 s-1 deg-2.

Export citation and abstract BibTeX RIS

Please wait… references are loading.
10.1086/321421