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- W1986598022 abstract "view Abstract Citations (25) References (15) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Mass Loss and the Formation of White-Dwarf Stars. Auer, L. H. ; Woolf, N. J. Abstract The presence of white dwarfs in the Hyades and a suspected one in the Pleiades indicate that stars with masses greater than 2 5 Mo, and possibly 7 Mo, can become white dwarfs Calculations show that the excess mass cannot be lost merely through rotational shedding if the star always rotates like a solid body. Consideration of wide pairs containing a white dwarf indicates that mass is probably lost on a time scale greater than 10 years. Nuclear fuel must be the major source of energy for mass ejection, although in the case of too massive stars it will be insufficient to eject enough mass to permit a stable white-dwarf configuration. it is noted that the minimum masses for helium and carbon burning are comparable with the observed mean mass of white dwarfs, indicating that mass loss continues until nuclear burning ceases. Publication: The Astrophysical Journal Pub Date: July 1965 DOI: 10.1086/148275 Bibcode: 1965ApJ...142..182A full text sources ADS | data products SIMBAD (7)" @default.
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- W1986598022 date "1965-07-01" @default.
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- W1986598022 title "Mass Loss and the Formation of White-Dwarf Stars." @default.
- W1986598022 doi "https://doi.org/10.1086/148275" @default.
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