Peremennye Zvezdy

Article in PDF
"Peremennye Zvezdy",
Prilozhenie
,
vol. 8, N 31 (2008)

New Semiregular Pulsating Stars

M. L. Kuzmin
Moscow, Russia

ISSN 2221–0474

Received:   17.06.2008;   accepted:   16.09.2008
(E-mail for contact: m@kuzmin.me)


#NameOtherCoord (J2000)TypeMaxMinSystemPeriodEpoch (JD)typeSpCommentL.CurveFind.ChartData
1 GSC 04485-0068622 49 02.26, +72 35 54.3SR11.011.45R652451323max Comm. 11.gifch1.gifNSVS 168648 NSVS 1388313
2 USNO-A2.0 1425-1509877923 27 05.41, +57 25 34.7SR12.012.4R77:2451513max Comm. 22.gifch2.gifNSVS 1522263 NSVS 3497726
3 GSC 04007-0149023 29 53.64, +56 50 21.9SR11.111.55R582451605max Comm. 33.gifch3.gifNSVS 1524101
4 TYC 4284 00955 123 36 30.52, +63 27 28.3SRA10.811.0R37.42451512max Comm. 44.gifch4.gifNSVS 1483403 NSVS 3545309

Comments:


1. J-H = 0.968 (2MASS).

2. IRAS 23247+5708. J-H = 1.103 (2MASS).

3. IRAS Z23275+5633. J-H = 1.114 (2MASS).

4. B-V = 1.456 (Tycho 2).

Remarks:
I announce the discovery of four new semiregular pulsating variable stars found in the public data release from the Northern Sky Variablity Survey (NSVS; Wozniak et al., 2004; see also 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



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