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- W2094125434 abstract "The rotational velocities of white dwarfs provide constraints for models of the final stages of stellar evolution. Due to the inapplicability of von Zeipl's theorem, theoretical profiles show that rotational effects for rapidly rotating white dwarfs are only evident for triangle-openlambda<7 A.The observational evidence for slowly rotating white dwarfs is summarized. A grid of slowly rotating model atmospheres has been calculated with effective temperatures from 13,000 K to 28,000 K. Fitting to observations yields upsilon sin i<60 km s/sup -1/ for 40 Eri B and upsilon sub i<70 km s/sup -1/ for W1346.The rotational effect on the lines is small: information can be obtained only for triangle-openlambda<1 A. Sharp H..beta.. line cores were produced in each model. This line offers the best possibility for detecting rotation in DA white dwarfs." @default.
- W2094125434 created "2016-06-24" @default.
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- W2094125434 date "1979-01-01" @default.
- W2094125434 modified "2023-09-27" @default.
- W2094125434 title "On some aspects of Balmer-line formation in rotating white dwarfs" @default.
- W2094125434 doi "https://doi.org/10.1086/156764" @default.
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