Article in PDF |
"Peremennye Zvezdy", Prilozhenie, vol. 8, N 14 (2008) |
ISSN 2221–0474 |
Received: 23.03.2008; accepted: 24.03.2008
(E-mail for contact: khruslov@bk.ru)
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Comments:
1. M-m = 0.1 P. J-H = 0.344 (2MASS). The ROTSE data with photometric correction flags (usually rejected) were kept for the analysis.
2. M-m = 0.45 P. J-H = 0.195 (2MASS). The ROTSE data with photometric correction flags (usually rejected) were kept for the analysis.
3. M-m = 0.45: P. J-H = 0.647 (2MASS).Remarks:
I present the discovery of 3 new pulsating 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:
Wozniak, P.R., Vestrand, W.T., Akerlof, C.W. et al., 2004, Astron. J., 127, 2436