Peremennye Zvezdy

Article in PDF
"Peremennye Zvezdy",
Prilozhenie
,
vol. 9, N 2 (2009)

Eight New RR Lyrae Variables

A. V. Khruslov
Russia, Tula

ISSN 2221–0474

Received:   29.01.2009;   accepted:   9.02.2009
(E-mail for contact: khruslov@bk.ru)


#NameOtherCoord (J2000)TypeMaxMinSystemPeriodEpoch (JD)typeSpCommentL.CurveFind.ChartData
1 GSC 2548-0025114 02 27.04, +34 17 45.1RRAB14.014.5R0.74272451423.900max Comm. 11.PNGchart1.PNGNSVS 7710384
2 GSC 4172-0021714 18 55.37, +62 02 57.6RRAB13.814.5R0.593232451429.822max Comm. 22.PNGchart2.PNGNSVS 2720898
3 GSC 3865-0126214 28 55.07, +57 30 23.9RRAB14.114.9R0.62012451406.956max Comm. 33.PNGchart3.PNGNSVS 2739793
4 TYC 3863 00740 114 41 38.24, +56 26 17.1RRC11.411.75R0.1976952451395.545max Comm. 44.PNGchart4.PNGNSVS 2743436
5 GSC 3860-0057914 41 54.89, +53 56 47.9RRAB14.115.2R0.45632451382.927max Comm. 55.PNGchart5.PNGNSVS 2743872 NSVS 5133533
6 GSC 3065-0206716 13 24.72, +41 09 48.5RRC:14.615.2R0.384642451374.520max Comm. 66.PNGchart6.PNGNSVS 5234294
7 GSC 2739-0053822 38 22.26, +32 38 54.6RRC13.8514.3R0.311682451434.701max Comm. 77.PNGchart7.PNGNSVS 8909981
8 GSC 2756-0046123 18 06.72, +32 12 36.4RRAB14.215.2R0.554852451447.592max Comm. 88.PNGchart8.PNGNSVS 9022293

Comments:


1. M-m = 0.25:P. J-H = 0.238 (2MASS).

2. M-m = 0.22P. J-H = 0.221 (2MASS). The ROTSE data with photometric correction flags (usually rejected) were kept for the analysis.

3. M-m = 0.18P. J-H = 0.374 (2MASS). The ROTSE data with photometric correction flags (usually rejected) were kept for the analysis.

4. M-m = 0.38P. J-H = 0.123 (2MASS), B-V = 0.049 (Tycho2).

5. M-m = 0.23P. J-H = 0.299 (2MASS). The ROTSE data with photometric correction flags (usually rejected) were kept for the analysis.

6. M-m = 0.35:P. J-H = 0.174 (2MASS).

7. M-m = 0.32P. J-H = 0.126 (2MASS).

8. M-m = 0.18P . J-H = 0.293 (2MASS). The ROTSE data with photometric correction flags (usually rejected) were kept for the analysis.

Remarks:
I present the discovery of eight new RR Lyrae 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



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