A Close Look at the Population of Supersoft and Quasi‐soft X‐Ray Sources Observed in M31 withXMM‐Newton-Reference-Cited by-同舟云学术

A Close Look at the Population of Supersoft and Quasi‐soft X‐Ray Sources Observed in M31 withXMM‐Newton

Published:2006-06 Issue:2 Volume:643 Page:844-862
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Orio Marina

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference85 articles.

1. Variable stars towards the bulge of M 31: The AGAPE catalogue

2. Arnaud, K. A. 1996, in ASP Conf. Ser. 101, Astronomical Data Analysis Software and Systems V, ed. G. H. Jacoby & A. Barnes (San Francisco: ASP), 17

3. The X‐Ray Spectral Evolution of Classical Nova V1974 Cygni 1992: A Reanalysis of theROSATData

4. The complex X-ray spectrum of the supersoft source

5. The Interstellar Medium of M31. II. A Survey of 20 Centimeter Continuum Emission

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