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Abstrakty
We report extensive photometry of the frequently outbursting dwarf nova RZ Leo Minoris. During two seasons of observations we detected 12 superoutbursts and 7 normal outbursts. The V magnitude of the star varied in range from 16.5 mag to 13.9 mag. The superoutbursts occur quite regularly flashing every 19.07(4) days and lasting slightly over 10 days. The average interval between two successive normal outbursts is 4.027(3) days. The mean superhump period observed during the superoutbursts is Psh=0.059396(4) days (85.530±0.006 min). The period of the superhumps was constant except for one superoutburst when it increased with a rate of P/Psh=7.6(1.9)×10-5. Our observations indicate that RZ LMi enters the stage of permanent superhumps, both in superoutbursts and quiescence. This may indicate that decoupling of thermal and tidal instabilities play important role in ER UMa systems. No periodic light variations which can be connected with orbital period of the binary were seen, thus the mass ratio and evolutionary status of RZ LMi are still unknown.
Słowa kluczowe
Czasopismo
Rocznik
Tom
Strony
131--152
Opis fizyczny
Bibliogr. 36 poz., 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
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
Bibliografia
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- Rutkowski, A., Olech, A.,Mularczyk, K., Boyd, D., Koff, R., and Wiśniewski,M. 2007, Acta Astron., 57, 267.
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Typ dokumentu
Bibliografia
Identyfikator YADDA
bwmeta1.element.baztech-b128bb5c-5c5d-4d80-af75-1e580099e810