Optical identification of supersoft X-ray sources in M31

Details Optical identification of supersoft X-ray sources in M31 Optical identification of supersoft X-ray sources in M31

2001-02-26

arxiv.org/abs/astro-ph/0102441v1

Astronomy and Astrophysics

Astrophysics

1 .tex file, 1.sty file, 1 .ps file (figure)

Scientific paper

We report on initial progress in a program of optical identification of supersoft X-ray sources in M31, pursued mainly with the WIYN telescope. We propose the identification of one supersoft X-ray source with a variable star, which we believe to have been a classical or recurrent nova in outburst in September 1990. The nova remnant must have been still a supersoft X-ray sources 5 years after this observation, when it was observed with ROSAT.

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