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We present the results of a photometric campaign of the dwarf nova V1040 Cen. The light curve shows two normal outbursts with recurrence time ≈40 days and amplitude ≈2.5 mag. Quiescence data show oscillations with periods in the range ≈0.1 days (2.4 h) to ≈0.5 days (12 h) of unknown origin. We measured the orbital period of V1040 Cen to be Porb=0.060458(80) days (1.451±0.002 h). Based on the MV-Porb relation we found the distance of V1040 Cen to be 137±31 pc. In this paper we also report the detection of eleven new variable stars in the field of the monitored dwarf nova.
Czasopismo
Rocznik
Tom
Strony
345--357
Opis fizyczny
bibliogr. 24 poz., rys., tab., wykr.
Twórcy
autor
- TUBITAK National Observatory, Akdeniz University Campus, 07058 Antalya, Turkey
autor
- Warsaw University Observatory, Al.Ujazdowskie 4, 00-478 Warsaw, Poland
autor
- Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, ul. Bartycka 18, 00-716 Warszawa, Poland
autor
- Istanbul University, Faculty of Sciences, Department of Astronomy and Space Sciences, 34119 University, Istanbul, Turkey
autor
- Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, ul. Bartycka 18, 00-716 Warszawa, Poland
autor
- Warsaw University Observatory, Al.Ujazdowskie 4, 00-478 Warsaw, Poland
autor
- Departamento de Fisica y Astrofisica, Universidad de Valparaiso, Av. Gran Bretaña 1111, Valparaiso, Chile
autor
- TUBITAK National Observatory, Akdeniz University Campus, 07058 Antalya, Turkey
- Akdeniz University, Faculty of Science and Art, Physics Department 07058 Campus, Antalya, Turkey
Bibliografia
- Ak, T., Bilir, S., Ak, S., and Eker, Z. 2008, New Astron., 13, 133.
- Ak, T., Bilir, S., and Retter, A. 2007, New Astron., 12, 446.
- Alard, C., and Lupton, R.H. 1998, ApJ, 503, 325.
- Cutri, R.M., et al. 2003, ViezieR On-Line Data Catalog, II/246, Orginally published in University of Massachusetts and Infrared Processing and Analysis Center.
- Kato, T., Nogami, D., Moilanen, M., and Yamaoka, H. 2003, PASJ, 55, 989.
- Knigge, C. 2006, MNRAS, 373, 484.
- Olech, A., et al. 2011, A&A, 532, A64.
- Olech, A., Rutkowski, A., and Schwarzenberg-Czerny, A. 2009, MNRAS, 399, 465.
- Osaki, Y. 1996, PASP, 108, 390.
- Paczyński, B., and Schwarzenberg-Czerny, A. 1980, Acta Astron., 30, 127.
- Patterson, J., et al. 2003, PASP, 115, 1308.
- Pretorius, M. L., and Knigge, C. 2008a, MNRAS, 385, 1471.
- Pretorius, M. L., and Knigge, C. 2008b, MNRAS, 385, 1485.
- Rutkowski, A., Olech, A., Poleski, R., Sobolewska, M., Kankiewicz, P., Ak, T., and Boyd, D. 2010, Acta Astron., 60, 337.
- Rutkowski, A., Olech, A., Wiśniewski, M., Pietrukowicz, P., Pala, J., and Poleski, R. 2009, A&A, 497, 437.
- Rutkowski, A., Olech, A., Mularczyk, K., Boyd, D., Koff, R., andWiśniewski,M. 2007, Acta Astron., 57, 267.
- Schlegel, D.J., Finkbeiner, D.P., and Davis, M. 1998, ApJ, 500, 525.
- Schwarzenberg-Czerny, A. 1996, ApJ, 460, L107.
- Smak, J. 2009, Acta Astron., 59, 121.
- Smak, J. 2010, Acta Astron., 60, 357.
- Stetson, P.B. 1987, PASP, 99, 191.
- Warner, B. 1995, “Cataclysmic Variable Stars”, Cambridge University Press.
- Woudt, P., and Warner, B. 2010, MNRAS, 403, 398.
- Woźniak, P.R. 2000, Acta Astron., 50, 421.
Typ dokumentu
Bibliografia
Identyfikator YADDA
bwmeta1.element.baztech-236d92af-1c99-4653-a5dd-0c4b58e037e4