Peremennye Zvezdy

Article in PDF
"Peremennye Zvezdy",
Prilozhenie
,
vol. 8, N 13 (2008)

New Variable Stars from NSVS. III

M. L. Kuzmin
Moscow, Russia

ISSN 2221–0474

Received:   19.03.2008;   accepted:   19.03.2008
(E-mail for contact: ml.kuzmin@gmail.com)


#NameOtherCoord (J2000)TypeMaxMinSystemPeriodEpoch (JD)typeSpCommentL.CurveFind.ChartData
1 GSC 04450-0030820 01 54.52, +70 12 29.9RRC13.3513.8R0.326712451560.934max  01.jpgch01.jpgNSVS 1228708 NSVS 1322661
2 GSC 04446-0098920 13 27.79, +67 52 25.5SRD11.812.05R75.22451574.5max Comm. 202.jpgch02.jpgNSVS 1323130 NSVS 3185646
3 GSC 04232-0057220 13 57.92, +61 24 18.6SR:10.811.25R69:2451600.5max  03.jpgch03.jpgNSVS 3181327
4 GSC 04247-0013920 55 26.11, +61 35 27.7RS12.212.4R5.80982451342.6max Comm. 404.jpgch04.jpgNSVS 3257349 NSVS 3307184
5 GSC 04251-0140921 01 37.61, +62 00 40.8EW12.612.95R0.452242451448.943min Comm. 505.jpgch05.jpgNSVS 3310908
6 GSC 03964-0000321 02 11.43, +59 53 19.0EW12.813.0R0.438062451475.581min Comm. 606.jpgch06.jpgNSVS 3262418
7 GSC 04598-0074121 14 22.80, +82 18 31.2RS12.512.85R5.1862451673.55max Comm. 707.jpgch07.jpgNSVS 35637 NSVS 1265108
8 GSC 04470-0010621 47 44.96, +72 57 46.4LB12.112.5R  other  08.jpgch08.jpgNSVS 1363335
9 GSC 04274-0170221 52 33.03, +65 47 34.4EB12.512.8R1.176522451277.661min Comm. 909.jpgch09.jpgNSVS 3339975 NSVS 3378585
10 GSC 04466-0028321 53 09.69, +70 49 23.6EB14.1514.75:R1.581812451502.447min Comm. 1010.jpgch10.jpgNSVS 1366062
11 GSC 02748-0099622 41 45.15, +37 07 16.0RRAB12.813.25R0.747512451397.85max  11.jpgch11.jpgNSVS 6117158 NSVS 8914671

Comments:


2. Not very red. J = 9.697, H = 9.096, K = 8.963 (2MASS).

4. 1RXS J205529.6+613509.

5. Min II = 12.9. Type RRC is not excluded (JD(max) = 2451511.899 + 0.2261 x E).

6. Min II = 13.0.

7. 1RXS J211416.9+821831.

9. Min II = 12.7.

10. Min II = 14.6.

Remarks:
I announce the discovery of 11 new 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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