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- W26902590 abstract "Theoretical continua (3000 ≲ λ (Å) ≲ 20000), UBV colours and Balmer absorption line profiles (Hα – Hδ) have been computed for the optically thick parts of steady-state accretion discs around white dwarfs as a function of mass flow rate, mass of white dwarf and inclination angle. The uncertainties due to disc z-structure and outer radius and viscosity are considered. The theoretical results for continua and UBV colours are compared with the theoretical results of Schwarzenberg-Czerny and Rózyczka (1977) and Herter et al . (1979) and with results obtained using black bodies instead of stellar atmospheres (e.g. Lynden-Bell 1969). Where models can be directly compared the quantitative agreement is good." @default.
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- W26902590 date "1979-08-01" @default.
- W26902590 modified "2023-09-23" @default.
- W26902590 title "Theory and Observations of Accretion Disc Spectra" @default.
- W26902590 cites W2078521163 @default.
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- W26902590 doi "https://doi.org/10.1017/s0252921100076296" @default.
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