Article in PDF |
"Peremennye Zvezdy", Prilozhenie, vol. 5, N 5 (2005) |
ISSN 2221–0474 |
Received: 10.11.2005; accepted: 13.12.2005
(E-mail for contact: khruslov@bk.ru)
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Remarks: |
NSV 855 was discovered by Wachmann (1939) and independently by Kinman et al. (1982),
the star's type was not determined. According to ROTSE-I data (Akerlof et al., 2000)
and
in agreement with photographic observations from Kinman et al. (1982), it is a HADS
(high-amplitude Delta Scuti) star with M-m = 0.23P (ROTSE-I) and M-m = 0.35P, range
13.3
- 13.8 (pg) (Kinman et al.). |
References: |
Akerlof, C., Amrose, S., Balsano, R. et al., 2000, AJ, 119, 1901
Kinman, T.D., Mahaffey, C.T., Wirtanen, C.A., 1982, AJ, 87, 314 Wachmann, A.A., 1939, Spektral-Durchmusterung von Milchstrassenfeldern, Teil 1 |
Light Curve The small dots in the bottom panel of the Figure are uncertain data points. |