Article in PDF |
"Peremennye Zvezdy", Prilozhenie, vol. 6, N 31 (2006) |
ISSN 2221–0474 |
Received: 13.11.2006; accepted: 28.11.2006
(E-mail for contact: khruslov@bk.ru)
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Comments:
1. M-m = 0.20 P.
2. M-m = 0.25 P.
3. M-m = 0.15 P.
5. M-m = 0.35 P. A one-day alias period, 0.27596 d, is not excluded.
6. M-m = 0.11 P.
7. M-m = 0.3: P.
8. M-m = 0.15 P. The ROTSE data with photometric correction flags (usually rejected) were kept for the analysis. In the case of GSC 4182-00914, the use of these data considerably increases the number of available observations without deteriorating quality and allows us to determine the period more accurately.
9. M-m = 0.1 P.
10. M-m = 0.2 P.Remarks:
I present the discovery of 10 new RR Lyrae 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 from the 2MASS catalog.References:
Wozniak, P.R., Vestrand, W.T., Akerlof, C.W. et al., 2004, Astron. J., 127, 2436