Infrared emission around Cyg X-3

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dc.creatorOgley, R. N.
dc.creatorBurnell, S. J. Bell
dc.creatorFender, R. P.
dc.date1996-09-17
dc.date.accessioned2026-07-07T02:21:55Z
dc.date.available2026-07-07T02:21:55Z
dc.descriptionWe present UKIRT infrared images of the X-ray binary Cygnus X-3. We address the possibility of extended infrared emission and show that it could be either warm circumstellar material or a star near the binary's line of sight.
dc.descriptionto appear in "Accretion Phenomena and Associated Outflows", IAU Coll. 163, Port Douglas, Australia, July 1996; 2 pages, 0 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/9609112
dc.identifierhttp://arxiv.org/abs/astro-ph/9609112
dc.identifierASP Conf Ser 121 (1997) 775
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10686
dc.subjectAstrophysics
dc.titleInfrared emission around Cyg X-3
dc.typetext

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