Optical identification of supersoft X-ray sources in M31

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dc.creatororio, Marina
dc.creatorCasalegno, Roberto
dc.creatorConselice, Chris
dc.creatorGreiner, Jochen
dc.creatorNedialkov, Petko L.
dc.creatorTikhonov, Nikolay A.
dc.date2001-02-26
dc.date.accessioned2026-07-07T01:57:49Z
dc.date.available2026-07-07T01:57:49Z
dc.descriptionWe 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.
dc.description1 .tex file, 1.sty file, 1 .ps file (figure)
dc.identifierhttps://arxiv.org/abs/astro-ph/0102441
dc.identifierhttp://arxiv.org/abs/astro-ph/0102441
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2536
dc.subjectAstrophysics
dc.titleOptical identification of supersoft X-ray sources in M31
dc.typetext

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