Article in PDF |
"Peremennye Zvezdy", Prilozhenie, vol. 9, N 15 (2009) |
ISSN 2221–0474 |
Received: 17.04.2009; accepted: 15.06.2009
(E-mail for contact: khruslov@bk.ru)
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Comments:
1. MinII = 11.23. The ROTSE data with photometric correction flags (usually rejected) were kept for the analysis.
2. MinII = 12.7.
3. MinII = 10.8.
4. MinII = 13.85. D = 0.13P.
5. MinII = 12.0. D = 0.15P.
6. MinII = 14.0.
7. MinII = 12.9. D = 0.10P. The author discovered this star independently. It was earlier announced by Hoffman et al. (2008), where a twice longer period was suggested.Remarks:
I present the discovery of seven new Eclipsing Binaries variables. A search for variables was carried out in the publicly available data of the Northern Sky Variability Survey (NSVS, Wozniak et al., 2004, also see http://skydot.lanl.gov/nsvs). These observations were analyzed using the period-search software developed by Dr. V.P. Goranskij for Windows environment. The coordinates were drawn either from the Tycho-2 or from the 2MASS catalogs.References:
Hoffman, D.I., Harrison, T.E., Coughlin, J.L. et al., 2008, Astron. J., 136, 1067
Wozniak, P.R., Vestrand, W.T., Akerlof, C.W. et al., 2004, Astron. J., 127, 2436