Article in PDF |
"Peremennye Zvezdy", Prilozhenie, vol. 6, N 8 (2006) |
ISSN 2221–0474 |
Received: 28.02.2006; accepted: 14.03.2006
(E-mail for contact: khruslov@bk.ru)
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Comments:
1. M-m = 0.35 P.
2. M-m = 0.18: P.
3. M-m = 0.1 P.
4. M-m = 0.2 P.
5. M-m = 0.1 P.
6. M-m = 0.13 P.
7. M-m = 0.11 P.
8. M-m = 0.12: P.
9. M-m = 0.12 P.
10. M-m = 0.15: P.
11. M-m = 0.35 P.
12. M-m = 0.2 P.
13. M-m = 0.35 P.
14. M-m = 0.35 P.
15. M-m = 0.3: P. The period 0.3371 d gives a much worse light curve.
16. M-m = 0.15: P.
17. M-m = 0.32 P.
18. M-m = 0.3 P.
19. M-m = 0.2 P.
20. M-m = 0.15 P.
21. M-m = 0.19 P.
22. M-m = 0.4 P.
23. M-m = 0.15 P.
24. M-m = 0.15: P.Remarks:
I present the discovery of 24 new RR Lyrae variables in Bootes, Camelopardalis, Draco and Hercules. 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