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We report extensive photometry of the dwarf nova KS UMa throughout its 2003 superoutburst till quiescence. During the superoutburst the star displayed clear superhumps with a mean period of Psh=0.070092(23) days. In the middle stage of superoutburst the period was increasing with a rate of P/P=(21±12)×10-5 and later was decreasing with a rate of P/P=-(21±8)×10-5. At the end of superoutburst and during first dozen days of quiescence the star was showing late superhumps with a mean period of Plate=0.06926(2) days. This phenomenon was observed even 30 days after beginning of the superoutburst. In quiescence the star shows quasi-periodic modulations with amplitude reaching 0.5 mag. The most common structure observed during this stage was sinusoidal wave characterized by a period of about 0.1 days. Comparing KS UMa to other SU UMa stars we conclude that this group of dwarf novae shows decreasing superhump periods at the beginning and the end of superoutburst but increasing period in the middle phase.
Słowa kluczowe
Czasopismo
Rocznik
Tom
Strony
175--194
Opis fizyczny
Bibliogr. 30 poz., rys., tab., wykr.
Twórcy
autor
- Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, ul. Bartycka 18, 00-716 Warszawa, Poland
autor
- Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, ul. Bartycka 18, 00-716 Warszawa, Poland
- Adam Mickiewicz University Observatory, ul. Słoneczna 36, 60-286 Poznań, Poland
autor
- Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warsaw, Poland
autor
- Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warsaw, Poland
autor
- Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warsaw, Poland
autor
- Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warsaw, Poland
Bibliografia
- Baba, H., Kato, T., Nogami, D., Hirata, R., Matsumoto, K., and Sadakane, K. 2000, PASJ, 52, 429.
- Balayan, S.K. 1997, Astrophys. J., 40, 101.
- Harvey, D.A., and Patterson, J. 1995, P.A.S.P., 107, 1055.
- Hazen, M.L., and Garnavich, P.M. 1999, JAAVSO, 27, 19.
- Howell, S.B., DeYoung, J.A., Mattei, J.A., Foster, G., Szkody, P., Cannizzo, J.K., Walker, G., and Fierce, E. 1996, Astron. J., 111, 2367.
- Kato, T., Kiyota, S., Novak, R., and Matsumoto, K. 1999, IBVS, No. 4794.
- Kato, T., Masumoto, K., Nogami, D., Morikawa, K., and Kiyota, S. 2001a, PASJ, 53, 893.
- Kato, T., Sekine, T., and Hirata, R. 2001b, PASJ, 53, 1191.
- Kato, T., et al. 2003a, MNRAS, 339, 861.
- Kato, T., Nogami D., and Masuda, S. 2003b, PASJ, 55, L7.
- Lubow, S.H. 1992, Astrophys. J., 401, 317.
- Markarian, B.E., and Stepanian, D.A. 1983, Astrofizika, 19, 639.
- Nogami, D., Masuda, S., and Kato, T. 1997, PASP, 109, 1114.
- Nogami, D., et al. 2003, Astron. Astrophys., in print (astro-ph/0302538).
- Olech, A. 1997, Acta Astron., 47, 281.
- Olech, A. 2003, Acta Astron., 53, 85.
- Paczyński, B. 1981, Acta Astron., 31, 1.
- Patterson, J., Bond, H.E., Grauer, A.D., Shafter, A.W., and Mattei, J.A. 1993, PASP, 105, 69.
- Patterson, J., Jablonski, F., Koen, C., O’Donoghue, D., and Skillman, D.R. 1995, PASP, 107, 1183.
- Patterson, J., et al. 1998, PASP, 110, 1290.
- Patterson, J., et al. 2002, PASP, 114, 721.
- Schwarzenberg-Czerny, A. 1996, Astrophys. J. Letters, 460, L107.
- Semeniuk, I., Olech, A., Kwast, T., and Nale˙zyty, M. 1997a, Acta Astron., 47, 201.
- Semeniuk, I., Nale˙zyty, M., Gembara, P., and Kwast, T. 1997b, Acta Astron., 47, 299.
- Snowden, S.L., et al. 1997, Astrophys. J., 454, 643.
- Stetson, P.B. 1987, PASP, 99, 191.
- Udalski, A., and Pych, W. 1992, Acta Astron., 42, 285.
- Uemura, M., et al. 2002, PASJ, 54, 599.
- Warner, B. 1985, in: “Interacting Binaries”, Ed. P.P. Eggelton and J.E. Pringle (Dordrecht: D. Reidel Publishing Company), p. 367.
- Warner, B. 1995, “Cataclysmic Variable Stars”, Cambridge University Press.
Typ dokumentu
Bibliografia
Identyfikator YADDA
bwmeta1.element.baztech-93f60427-431c-48cb-a582-e559b64216db