Supersoft X‐Ray Sources in M31. I. AChandraSurvey and an Extension to Quasi‐soft Sources-Reference-Cited by-同舟云学术

Supersoft X‐Ray Sources in M31. I. AChandraSurvey and an Extension to Quasi‐soft Sources

Published:2004-07-20 Issue:1 Volume:610 Page:247-260
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Di Stefano R.,Kong A. K. H.,Greiner J.,Primini F. A.,Garcia M. R.,Barmby P.,Massey P.,Hodge P. W.,Williams B. F.,Murray S. S.,Curry S.,Russo T. A.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/610/i=1/a=247/pdf

Reference54 articles.

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2. Di Stefano, R., Friedman, R., Kundu, A. & Kong, A. K. H. 2004a, ApJL, submitted (astro-ph/0312391)

3. Di Stefano, R., Greiner, J., Kong, A., Garcia, M. R., Primini, F. A., Barmby, P., Murray, S. S. & Curry, S. 2002a, Poster presented at the American Physical Society April meeting, abstract N17.072

4. A New Way to Detect Massive Black Holes in Galaxies: The Stellar Remnants of Tidal Disruption

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