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: http://www.astronet.ru/db/varstars/msg/1223708
Дата изменения: Fri Nov 16 17:30:56 2007 Дата индексирования: Wed Dec 26 19:50:25 2007 Кодировка: Поисковые слова: messenger |
Received: 4.10.2007; accepted: 16.11.2007
(E-mail for contact: idkfa@sai.msu.ru)
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Remarks: | ||||||||||||||||||||||||||||||
V435 Cas was discovered as a variable star by Hoffmeister (1967). He
classified it as an eclipsing binary of Algol type and listed two times of
minima (see the table below). Six more times of minima were published by
Rosino,
Bianchini & di Martino (1976); despite that, the period of V435 Cas could not be
determined.
About 50 years after its discovery, V435 Cas was observed by the Optical Monitoring Camera (Mas-Hesse et al., 2003) on board the INTEGRAL satellite (Winkler et al., 2003). These observations are available via the OMC Data Server (Gutierrez et al., 2004). INTEGRAL/OMC data are presented in the form of FITS tables which were converted to ASCII format, used by our period-search software, by means of a custom-made convertor (its source code is available at ftp://scan.sai.msu.ru/pub/software/OMC2ASCII ). The well-sampled (1025 data points) V-band light curve combined with information on times of minima observed in the 20th century lead to the following linear light elements: HJDmin = 2453404.887 + 4.156074 x E.
Note that the Simbad database, as of November, 2007, returns a wrong position for V435 Cas, based on the identification by Kato (1999). The correct position, in agreement with the discoverer's finding chart (Hoffmeister, 1967), was given by Skiff (1997) and can be found through the GCVS website. The position of the source IOMC 4011000047 (= V435 Cas), observed by INTEGRAL, confirms the GCVS identification. Acknowledgments: This research is based on data from the OMC Archive at LAEFF, pre-processed by ISDC. The author has made use of the Aladin Sky Atlas (Bonnarel et al., 2000), the International Variable Star Index, the O-C gateway created by A. Paschke and L. Brat, the period search software developed by V.P. Goranskij. | ||||||||||||||||||||||||||||||
References: | ||||||||||||||||||||||||||||||
Bonnarel, F., Fernique, P., Bienayme, O., et al., 2000, A&AS, 143, 33
Gutierrez, R., Solano, E., Domingo, A., Garcia, J., 2004, ASP Conference Series, 314, 153 Hoffmeister, C., 1967, AN, 290, 43 Kato, T., 1999, IBVS, No. 4789 Mas-Hesse, J. M., Gimenez, A., Culhane, J.L., et al., 2003, A&A, 411, L261 Rosino, L., Bianchini, A., di Martino, D., 1976, A&AS, 24, 1 Skiff, B.A., 1997, IBVS, No. 4441 Winkler, C., Courvoisier, T.J-L., Di Cocco, G., et al., 2003, A&A, 411, L1 |
Light Curve![]() Finding Chart ![]() A POSS-II red image centered on V435 Cas. Data Source |