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Curious Variables Experiment (CURVE). RZ LMi - the Most Active SU UMa Star

Wybrane pełne teksty z tego czasopisma
Identyfikatory
Warianty tytułu
Języki publikacji
EN
Abstrakty
EN
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.
Czasopismo
Rocznik
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
  • Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, ul. Bartycka 18, 00-716 Warszawa, Poland
  • 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
  • Warsaw University Observatory, Al. Ujazdowskie 4, 00-476 Warszawa, Poland
Bibliografia
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  • Henden, A.A., and Honeycutt, R.K. 1995, PASP, 107, 324.
  • Ishioka, R., Kato, T., Uemura, M., Iwamatsu, H., Matsumoto, K., Martin, B.E., Billings, G.W., and Novak, R. 2001, PASJ, 53, L51.
  • Kato, T., Nogami, D., and Baba, H. 1996, PASJ, 48, L93.
  • Kato, T. 2001, PASJ, 53, L17.
  • Kato, T., Nogami, D., and Masuda, S. 2003, PASJ, 55, L7.
  • Lipovetskij, V., and Stepanjan, J. 1981, Astrophysics, 17, 573.
  • Misslet, K.A., and Shafter, A.W. 1995, AJ, 109, 1757.
  • Nogami, D., Kato, T., Masuda, S., Hirata, R., Matsumoto, K., Tanabe, K., and Yokoo, T. 1995, PASJ, 47, 897.
  • Olech, A., Schwarzenberg-Czerny, A., Kędzierski, P., Złoczewski, K., Mularczyk, K., and Wiśniewski, M. 2003a, Acta Astron., 53, 175.
  • Olech, A., Złoczewski, K., Mularczyk, K., Kędzierski, P., Wiśniewski, M., and Stachowski, G. 2004, Acta Astron., 54, 57.
  • Olech, A., Mularczyk, K., Kędzierski, P., Złoczewski, K., Wiśniewski, M., and Szaruga, K. 2006, A&A, 2006, 933.
  • Olech, A., Rutkowski, A., and Schwarzenberg-Czerny, A. 2007, Acta Astron., 57, 331.
  • Osaki, Y. 1995, PASJ, 47, L11.
  • Osaki, Y. 1996, PASP, 108, 39.
  • Patterson, J., Jablonski, F., Koen, C., O’Donoghue, D., and Skillman, D.R. 1995, PASP, 107, 1183.
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  • Patterson, J. 2001, PASP, 113, 736.
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  • Robertson, J.W., Honeycutt, R.K., and Turner, G.W. 1995, PASP, 107, 443.
  • Rutkowski, A., Olech, A.,Mularczyk, K., Boyd, D., Koff, R., and Wiśniewski,M. 2007, Acta Astron., 57, 267.
  • Schreiber, M.R, and Lasota, J.-P. 2007, A&A, 473, 897.
  • Schwarzenberg-Czerny, A. 1996, ApJ, 460, L107.
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Typ dokumentu
Bibliografia
Identyfikator YADDA
bwmeta1.element.baztech-b128bb5c-5c5d-4d80-af75-1e580099e810
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