Abstract
Upper bounds to the masses of He envelopes of white dwarfs are derived by examining the maximum He envelope that a nucleus of a planetary nebulae can have consistent with observation.
Original language | English |
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Pages (from-to) | 385-390 |
Number of pages | 6 |
Journal | Astrophysics and Space Science |
Volume | 23 |
Issue number | 2 |
DOIs | |
State | Published - Aug 1973 |