Time-resolved photometry of cataclysmic variables

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dc.creatorPapadaki, C.
dc.creatorBoffin, H. M. J.
dc.creatorCuypers, J.
dc.creatorStanishev, V.
dc.creatorKraicheva, Z.
dc.creatorGenkov, V.
dc.date2003-12-18
dc.date.accessioned2026-07-07T02:11:38Z
dc.date.available2026-07-07T02:11:38Z
dc.descriptionWe present time-resolved photometry of two cataclysmic variables whose CCD photometric observations were obtained with the 1m telescope at the South African Astronomical Observatory in October 2002 and August 2003 and with the 1m telescope at Hoher List in Germany. Concerning MCT 2347-3144 we detect for the first time a period of 6.65h. For V1193 Ori the 3.96 h periodicity has for the first time been confirmed through time-resolved photometry.
dc.descriptionConference Proceedings of the Oct. 2003 Workshop "Spectroscopically and Spatially Resolving the Components of Close Binary Stars"
dc.identifierhttps://arxiv.org/abs/astro-ph/0312477
dc.identifierhttp://arxiv.org/abs/astro-ph/0312477
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7162
dc.subjectAstrophysics
dc.titleTime-resolved photometry of cataclysmic variables
dc.typetext

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