Identyfikatory
Warianty tytułu
Języki publikacji
Abstrakty
Disk eclipse light curves of UX UMa and RW Tri are reanalyzed in order to determine two parameters: d log M/d log R, which is a measure of systematic deviations from stationary accretion, and Δlog Tedgeedge, which is a correction to the temperature of the disk's edge. For both systems the resulting values of d log M/d log R are slightly negative, most likely due to irradiation of the innermost parts of the disk by the boundary layer. Taking this into account we conclude that accretion in UX UMa and RW Tri is indeed stationary. For both systems there is no evidence for Δlog T_edge being significantly different from zero. Our results contradict those obtained earlier with the MEM technique by Horne and Stiening (1985) and Rutten et al. (1992), which showed the accretion rate to be a strongly increasing function of the radial distance. This means that even at moderate inclinations (i=73.0 and 70.5 degrees) the MEM technique produces spurious results.
Czasopismo
Rocznik
Tom
Strony
59--63
Opis fizyczny
Bibliogr. 11 poz., tab.
Twórcy
autor
- N. Copernicus Astronomical Center, Polish Academy of Sciences, ul. Bartycka 18, 00-716 Warsaw, Poland
Bibliografia
- Horne, K. 1993, "Accretion Disks in Compact Stellar Systems", ed. J.C. Wheeler, Singapore: World Scientific, p. 117.
- Horne, K., and Stiening, R.F. 1985, MNRAS, 216, 933.
- Johnson, H.L., Perkins, B., and Hiltner, W.A. 1954, Astrophys. J. Suppl. Ser., 1, 91.
- Rutten, R.G.M., van Paradijs, J., and Tinbergen, J. 1992, Astron. Astrophys., 260, 213.
- Smak, J. 1989, Acta Astron., 39, 201.
- Smak, J. 1994a, Acta Astron., 44, 45.
- Smak, J. 1994b, Acta Astron., 44, 59.
- Smak, J. 1994c, Acta Astron., 44, 265.
- Smak, J. 1995, Acta Astron., 45, 259.
- Walker, M.F., and Herbig, G.H. 1954, Astrophys. J., 120, 337.
- Warner, B. 1995, "Cataclysmic Variable Stars", Cambridge University Press.
Typ dokumentu
Bibliografia
Identyfikator YADDA
bwmeta1.element.baztech-65df0bf1-fcdd-44cd-82b3-4fb891827758