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Języki publikacji
Abstrakty
Model calculations describing the flow of material heated by irradiation into the shadow zone around L1 are described. In dwarf novae with very short periods (P≈1-2 hrs) the resulting enhancement in the mass outflow rate is very large: M/M0≈10-30. In systems with periods just above the period gap (P≈4 hrs) the enhancement is smaller: M/M0≈2-6. In systems with longer periods (P≈6 hrs), however, it turns out that the flow does not reach the vicinity of L1 and, consequently, the enhancement is negligibly small. This means that irradiation induced enhanced mass outflow plays important role in SU UMa stars but is negligible in Z Cam stars.
Słowa kluczowe
Czasopismo
Rocznik
Tom
Strony
181--193
Opis fizyczny
Bibliogr. 17 poz., rys., tab., wykr.
Twórcy
autor
- N. Copernicus Astronomical Center, Polish Academy of Sciences, Bartycka 18, 00-716 Warsaw, Poland
Bibliografia
- Hameury, J.M., King, A.R., and Lasota, J.P. 1988, Astron. Astrophys., 192, 187.
- King, A.R. 1989, MNRAS, 241, 365.
- Kovetz, A., Prialnik, D., and Shara, M.M. 1988, Astrophys. J., 325, 828.
- Marsh, T.R., and Horne, K. 1990, Astrophys. J., 349, 593.
- Meyer, F., and Meyer-Hofmeister, E. 1983, Astron. Astrophys., 121, 29.
- Milne, E.A. 1930, Handbuch der Astrophysik, 3, Part 1, 134.
- Osaki, Y. 1985, Astron. Astrophys., 144, 369.
- Osaki, Y. 1996, P.A.S.P., 108, 39.
- Osaki, Y., and Meyer, F. 2003, Astron. Astrophys., 401, 325.
- Ritter, H., and Kolb, U. 1998, Astron. Astrophys. Suppl. Ser., 129, 83.
- Robinson, E.L., Zhang, E.-H., and Stover, R.J. 1986, Astrophys. J., 305, 732.
- Sion, E.M. 1999, P.A.S.P., 111, 532.
- Smak, J. 1995, Acta Astron., 45, 355.
- Smak, J. 1998, Acta Astron., 48, 677.
- Smak, J. 2000, New Astronomy Reviews, 44, 171.
- Vogt, N. 1983, Astron. Astrophys., 118, 95.
- Warner, B. 1995, "Cataclysmic Variable Stars", Cambridge University Press.
Typ dokumentu
Bibliografia
Identyfikator YADDA
bwmeta1.element.baztech-9e4389fb-b79d-4486-8515-93622e063c8f