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- W1676948605 abstract "Abstract We present results of thermal and vibrational stability analysis for 1 M ⊙ white dwarf models corresponding to various accretion rates ≳ 10 −11 M ⊙ /y. Accretion is assumed to be spherically symmetric and stationary. Thermal instability due to nuclear burning of hydrogen (at lower accretion rates) and helium (at higher rates) was found. At medium rates two growing thermal modes are simultaneously present. Vibrational instability was found for all models except those corresponding to highest accretion rates. The excitation rates for some nonradial g-modes are at least 3 orders of magnitude higher than those for radial pulsations. These rates are also higher than the excitation rates for thermal modes in certain range of accretion rates corresponding to high luminosities and effective temperatures. Among objects in which these instabilities may be important are symbiotic stars and nuclei of planetary nebulae." @default.
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- W1676948605 date "1977-01-01" @default.
- W1676948605 modified "2023-09-25" @default.
- W1676948605 title "Stability of Accreting White Dwarfs in Close Binary Systems" @default.
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- W1676948605 doi "https://doi.org/10.1017/s0252921100069517" @default.
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