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- W2064514665 abstract "view Abstract Citations (24) References (26) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Convective mixing in helium white dwarfs. Vauclair, G. ; Fontaine, G. Abstract The conditions under which convective mixing episodes take place between the helium envelopes and the underlying carbon layers in helium-rich white dwarfs are investigated. It is found that, for essentially any value of the initial helium content less than the maximum mass a helium convection zone can have, mixing does occur and leads, in the vast majority of cases, to an almost pure carbon superficial composition. Mixing products that show only traces of carbon while retaining helium-dominated envelopes are possible only if the initial helium content is quite close to the maximum possible mass of the helium convection zone. In the presence of turbulence, this restriction could be relaxed, however, and the helium-rich 4670-A stars may possibly be explained in this fashion. Publication: The Astrophysical Journal Pub Date: June 1979 DOI: 10.1086/157113 Bibcode: 1979ApJ...230..563V Keywords: Convective Flow; Helium; Stellar Atmospheres; Turbulent Mixing; White Dwarf Stars; Carbon; Stellar Envelopes; Stellar Models; Astrophysics; Convection:White Dwarfs full text sources ADS |" @default.
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- W2064514665 date "1979-06-01" @default.
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- W2064514665 title "Convective mixing in helium white dwarfs" @default.
- W2064514665 doi "https://doi.org/10.1086/157113" @default.
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