Документ взят из кэша поисковой машины. Адрес оригинального документа : http://www.astronet.ru/db/varstars/msg/1247548
Дата изменения: Wed Aug 18 23:49:04 1971
Дата индексирования: Sat Feb 12 08:40:35 2011
Кодировка:

Поисковые слова: cygnus
Journal "Peremennye Zvezdy"
Peremennye Zvezdy

"Peremennye Zvezdy",
Prilozhenie
,
vol. 10, N 30 (2010)

Discovery of Variability for NOMAD-1 1127-0027360

V. V. Krushinsky, I. S. Zalozhnih, A. A. Popov, E. A. Avvakumova
Kourovka Astronomical Observatory and Ural State University, Ekaterinburg, Russia

Received:   14.10.2010;   accepted:   22.11.2010
(E-mail for contact: Ekaterina.Avvakumova@usu.ru)


Star Name: NOMAD-1 1127-0027360
Coordinates (J2000): 1 48 50.13, +22 46 37.4
Variability type: EB:;   Limits, System: 15.32 - 16.25 (I); 16.2 - 17.61 (R);    
Period: 0.320 d;   Epoch(min): JD 2455441.2871

Remarks:
The variability of NOMAD-1 1127-0027360 was discovered on frames obtained during observations of the gamma-ray burst GRB100901a with telescopes of the MASTER robotic net (Lipunov et al. 2010) (Tunka Valley; Kourovka astronomical observatory; Kislovodsk solar station) on September 1 - 2, 2010. Completely identical MASTER II telescopes, each of them consisting of two parallel optical telescopes on the same mount (40 cm aperture, 1:2.5 focal ratio), are installed at all three locations. They permit to take two simultaneous images in broadband filters. The telescopes are equipped with Apogee Alta U16 CCD cameras (Kodak KAF16000 chip, Peltier cooled). Additional observations of the object were carried out at Kourovka astronomical observatory on September 2 - 4, 2010. Instrumental I and R filters were used.

The reductions of CCD frames were carried out with the IRAF package (Tody 1993). We did not transform our observations to a standart photometric system. Our I-band observations cover both the primary and the secondary minimum as well as both maxima. The secondary maximum was not covered with our R-band observations. We suggest that the star is an EB eclipsing variable.

The period was determined using the FAMIAS software package developed in the framework of the FP6 European Coordination Action HELAS (Zima 2008).

This study was financially supported by the State Agency for Science and Innovation of the Ministry of Education and Science of the Russian Federation (state contract No. 02.740.11.0249).

References:
Lipunov, V., Kornilov, V., Gorbovskoy, E., et al., 2010, Advances in Astronomy, 2010, Article ID 349171
Tody, D., 1993, A.S.P. Conference Ser., 52, 173
Zima, W., 2008, Comm. in Asteroseismology, 155, 17

Light Curve
Discovery of Variability for NOMAD-1 1127-0027360
The I-band light curve.
Finding Chart
Discovery of Variability for NOMAD-1 1127-0027360
Data Source
  1. data.txt


Main Page | Search
Astronet | SAI | INASAN

Report problems