Time-resolved photometry of cataclysmic variables

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We 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.
Conference Proceedings of the Oct. 2003 Workshop "Spectroscopically and Spatially Resolving the Components of Close Binary Stars"

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Astrophysics

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http://salesiana.dossiersoluciones.com/handle/123456789/7162

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/astro-ph/0312477
 http://arxiv.org/abs/astro-ph/0312477

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arXiv