Article in PDF |
"Peremennye Zvezdy", Prilozhenie, vol. 10, N 18 (2010) |
ISSN 2221–0474 |
Received: 14.03.2010; accepted: 24.05.2010
(E-mail for contact: khruslov@bk.ru)
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Comments:
1. MinII = 11.35, D = 0.07 P. X-ray source 1RXS J000618.5+694817.
2. Twice shorter period and type RRC are possible. MinII = 13.35. The ROTSE data with photometric correction flags (usually rejected) were kept for the analysis.
3. MinII = 13.5. The ROTSE data with photometric correction flags (usually rejected) were kept for the analysis.
4. MinII = 13.2. The ROTSE data with photometric correction flags (usually rejected) were kept for the analysis.
5. MinII = 14.9. The ROTSE data with photometric correction flags (usually rejected) were kept for the analysis.
6. MinII = 11.9. The ROTSE data with photometric correction flags (usually rejected) were kept for the analysis.
7. MinII = 13.8. Faint close companion 2MASS 06100589+6959121 .
8. MinII = 14.5. A fainter close companion GSC 4407-00850, the amplitude of variability is underestimated.
9. D = 0.16 P. X-ray sources 1WGA J1333.3+5030 = XBS J133321.2+503102. Identification with the X-ray source 1RXS J133318.5+503105 is possible.
10. MinII = 13.35:, D = 0.12 P. O'Connell effect.
11. MinII = 14.0. The ROTSE data with photometric correction flags (usually rejected) were kept for the analysis.
12. MinII = 12.8, D = 0.16 P. Faint close companion GSC 2755-01037, the NSVS amplitude is slightly underestimated. Identification with the X-ray source 1RXS J230903.5+324634 is not excluded.
13. MinII = 11.82. Period P = 0.3632 days is not excluded. The ROTSE data with photometric correction flags (usually rejected) were kept for the analysis.
14. MinII = 14.6.Remarks:
I present the discovery of 14 new eclipsing binaries. 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 2MASS catalogs.References:
Wozniak, P.R., Vestrand, W.T., Akerlof, C.W., et al., 2004, Astron. J., 127, 2436