Peremennye Zvezdy

Article in PDF
"Peremennye Zvezdy",
Prilozhenie
,
vol. 6, N 31 (2006)

New RR Lyrae Variables II

A. V. Khruslov
Russia, Tula

ISSN 2221–0474

Received:   13.11.2006;   accepted:   28.11.2006
(E-mail for contact: khruslov@bk.ru)


#NameOtherCoord (J2000)TypeMaxMinSystemPeriodEpoch (JD)typeSpCommentL.CurveFind.ChartData
1 GSC 4352-0072905 52 46.50, +72 51 15.9RR12.813.1R0.427202451521.899max Comm. 11.pngchart1.pngNSVS 652422
2 GSC 4367-0103007 02 18.13, +72 08 52.6RRAB13.914.4R0.62822451526.64max Comm. 22.pngchart2.pngNSVS 672345
3 GSC 3028-0046713 31 15.85, +40 56 56.8RRAB14.415.3R0.514232451422.846max Comm. 33.pngchart3.pngNSVS 5084141
4 GSC2.2 N1303030914813 48 42.53, +41 55 07.9RRAB14.515.9R0.54512451396.56max  4.pngchart4.pngNSVS 5090133
5 GSC 3035-0093714 14 57.39, +39 19 23.9RRC:14.415.0R0.381072451395.565max Comm. 55.pngchart5.pngNSVS 5099579
6 GSC 3487-0068515 04 27.36, +51 52 04.2RRAB13.414.6R0.479502451391.783max Comm. 66.pngchart6.pngNSVS 5140510
7 GSC 3059-0066415 33 20.37, +43 44 27.2RR14.615.6R0.57052451387.87max Comm. 77.pngchart7.pngNSVS 5167763
8 GSC 4182-0091415 40 40.67, +60 48 24.3RRAB13.514.2R0.631142451409.653max Comm. 88.pngchart8.pngNSVS 2792535 NSVS 2812099
9 GSC 3520-0101517 18 21.88, +51 17 32.3RRAB14.315.4R0.606242451388.675max Comm. 99.pngchart9.pngNSVS 5308842
10 GSC 3521-0103317 32 23.75, +51 40 47.3RRAB12.613.6R0.43762451408.805max Comm. 1010.pngchart10.pngNSVS 5316661

Comments:


1. M-m = 0.20 P.

2. M-m = 0.25 P.

3. M-m = 0.15 P.

5. M-m = 0.35 P. A one-day alias period, 0.27596 d, is not excluded.

6. M-m = 0.11 P.

7. M-m = 0.3: P.

8. M-m = 0.15 P. The ROTSE data with photometric correction flags (usually rejected) were kept for the analysis. In the case of GSC 4182-00914, the use of these data considerably increases the number of available observations without deteriorating quality and allows us to determine the period more accurately.

9. M-m = 0.1 P.

10. M-m = 0.2 P.

Remarks:
I present the discovery of 10 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 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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