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Abstrakty
High speed BVR(I)C photometry of the short period RS CVn binary SV Cam is presented. Its light curve is asymmetric with a depression of brightness by 0.04-0.05 mag after the primary eclipse. Good fit of the synthetic light curve to the observational data in all colors can be obtained assuming presence of two cool spots with equal angular sizes of 20° and temperatures 4350 K located at middle latitude above and below the stellar equator on opposite hemispheres of the primary star.
Słowa kluczowe
Czasopismo
Rocznik
Tom
Strony
517--528
Opis fizyczny
Bibliogr. 30 poz., rys., wykr.
Twórcy
autor
- Shoumen University, 9700 Shoumen, Bulgaria
autor
- Shoumen University, 9700 Shoumen, Bulgaria
autor
- Cracow Pedagogical University, 30-084 Cracow, Podchorążych 2, Poland
- N. Copernicus Astronomical Center, 00-716 Warsaw, Bartycka 18, Poland
Bibliografia
- Agrawal, P.C., Riegler, G.R., and Garmire, G.P. 1980, MNRAS, 192, 725.
- Bradstreet, D. 1993, in: ”Light Curve Modeling of Eclipsing Binary Stars”, Ed. E. Milone (Springer-Verlag New York) p. 151.
- Budding, E., and Zeilik, M. 1986, in: ”Cool Stars, Stellar Systems, and The Sun, Ed. M. Zeilik and D. Gibson (Heidelberg, Springer-Verlag), p. 290.
- Budding, E., and Zeilik, M. 1987, Astrophys. J., 319, 827.
- Buren, D., and Young, A. 1985, Astrophys. J. Letters, 295, L39.
- Busso, M., and Scaltriti, F. 1985, Astron. Astrophys., 148, 29.
- Cellino, A., Scaltriti, F., and Busso, M. 1985, Astron. Astrophys., 144, 315.
- Djurasevic, G. 1998, Astron. Astrophys. Suppl. Ser., 127, 233.
- Frieboes-Conde, H., and Herczeg, T. 1973, Astron. Astrophys. Suppl. Ser., 12, 1.
- Hall, D. 1976, in" IAU Collquim 29, ”Multiple Periodic Variable Stars”, Ed. W. Fitch (Dordrecht, Reidel), p. 287.
- Hall, D. 1995, Proceedings of the 176th Symp. of the IAU, Ed. K. Strassmeier and J. Linski, Kluwer Acad. Publisher, p. 217.
- Hilditch, R., Harland, D., and McLean, B. 1979, MNRAS, 187, 797.
- Hill, G., and Rucinski, S. 1993, in: ”Light Curve Modeling of Eclipsing Binary Stars”, Ed. E.Milone, Springer-Verlag: New York, p. 135.
- Kim, T., et al. 1985, Publ. Korean Nat’l Astron. Obs., 7, 1.
- Kreiner, J., et al. 1993, IAU Coll No 136, ”Poster Papers on Stellar Photometry”, Ed. I. Elliot and C. Butler, Dublin Institute for Advanced Studies, p. 80.
- Krzesiński, J., and Wojcik, K. 1993, Astron. Astrophys., 280, 338.
- Kwee, K., and van Woerden, H. 1956, Bull. Astron. Inst. Neth., 12, 327.
- Mallama, A. 1980, Astrophys. J. Suppl. Ser., 44, 241.
- Milano, L. 1981, in" ”Photometric and Spectroscopic Binary Systems”, Ed. E. Carling and Z. Kopal (Dordrecht, Reidel), p. 331.
- Patkos, L. 1982a, Comm. Konkoly Obs., No 80.
- Patkos, L. 1982b, in: ”Ejection and Accretion of Matter in Binary Systems, ed. J. Tremko (Bratislava, VEDA), p. 61.
- Patkos, L., and Hempelman, A. 1994, Astron. Astrophys., 292, 119.
- Pojmański, G. 1998, Acta Astron., 48, 711.
- Rahunen, T., and Vilhu, O. 1982, IAU Colloquium 69, ”Binary and Multiiple stars as Tracers of Stellar Evolution”, Ed. Kopal Z. and Rahe J. (Dordrecht, Reidel), p. 289.
- Singh, K.P., Drake, S.A., and White, N.E. 1996, Astron. J., 111, 2415.
- Udalski, A. 1991, PhD Thesis.
- Vogt, S. 1981, Astrophys. J., 247, 975.
- Welty, A., and Ramsey, L. 1995, Astron. J., 109, 2187.
- Wilson, R., and Devinney E. 1971, Astrophys. J., 166, 605.
- Zeilik, M., De Blasi, S., and Rhodes, M. 1988, Astrophys. J., 332, 293.
Typ dokumentu
Bibliografia
Identyfikator YADDA
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