Peremennye Zvezdy

Article in PDF
"Peremennye Zvezdy",
Prilozhenie
,
vol. 6, N 17 (2006)

Discovery of Three New Cepheids

A. V. Khruslov, S. V. Antipin
(1)Russia, Tula ; (2)Sternberg Astronomical Institute and Institute of Astronomy, Russian Academy of Sciences, Moscow, Russia

ISSN 2221–0474

Received:   23.06.2006;   accepted:   28.06.2006
(E-mail for contact: khruslov@bk.ru , antipin@sai.msu.ru)


#NameOtherCoord (J2000)TypeMaxMinSystemPeriodEpoch (JD)typeSpCommentL.CurveFind.ChartData
1 GSC 3709-0075203 04 08.81, +57 17 53.7DCEPS12.7513.05R3.0582451505.10max Comm. 11.gifchart1.gifNSVS 1942726
2 GSC2.2 N31220012283203 20 14.32, +55 06 57.1DCEP13.213.6R4.412451463.03max Comm. 22.gifchart2.gifNSVS 1956729
3 TYC 3728 01350 103 34 23.73, +58 24 50.0DCEPS9.629.88R3.68182451479.64max Comm. 33.gifchart3.gifNSVS 1965376

Comments:


1. M-m = 0.45 P, b = -1.1 deg.

2. M-m = 0.33 P, b = -1.8 deg.

3. M-m = 0.5: P, b = +2.0 deg., B-V = 1.72

Remarks:
We present the discovery of 3 new Sepheid (DCEP and DCEPS) 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 2MASS catalogs.

References:
Wozniak, P.R., Vestrand, W.T., Akerlof, C.W. et al., 2004, Astron. J., 127, 2436



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