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We report extensive multi-station photometry of TT Boo during its June 2004 superoutburst. The amplitude of the superoutburst was about 5.5 mag and its length about 22 days. The star showed a small re-brightening starting around the 9th day of the superoutburst. During entire bright state we observed clear superhumps with amplitudes from 0.07 mag to 0.26 mag and a mean period of Psh=0.0779589(47) days (112.261±0.007 min). The period was not constant but decreased at the beginning and the end of superoutburst and increased in the middle phase. We argue that the complicated shape of the O-C diagram is caused by real period changes rather than by phase shifts. Combining the data from two superoutbursts, 1989 and 2004, allowed us to trace the birth of the late superhumps and we conclude that it is a rather quick process lasting about one day.
Słowa kluczowe
Czasopismo
Rocznik
Tom
Strony
233--247
Opis fizyczny
Bibliogr. 29 poz., tab., wykr.
Twórcy
autor
- Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, ul. Bartycka 18, 00-716 Warszawa, Poland
autor
- Center for Backyard Astrophysics (Concord), 1730 Helix Court, Concord, CA 94518, USA
autor
- Warsaw University Observatory, Al. Ujazdowskie 4, 00-476 Warszawa, Poland
autor
- Warsaw University Observatory, Al. Ujazdowskie 4, 00-476 Warszawa, Poland
autor
- Warsaw University Observatory, Al. Ujazdowskie 4, 00-476 Warszawa, Poland
autor
- Warsaw University Observatory, Al. Ujazdowskie 4, 00-476 Warszawa, Poland
autor
- Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, ul. Bartycka 18, 00-716 Warszawa, Poland
Bibliografia
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- Kato, T., Nogami, D., Moilanen, M., and Yamaoka, H. 2003a, PASJ, 55, 989.
- Kato, T., et al. 2003b, MNRAS, 339, 861.
- Kholopov, P.N., et al. 1998, “Combined General Catalogue of Variable Stars”, 4.1 Ed (II/214A).
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Typ dokumentu
Bibliografia
Identyfikator YADDA
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