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 |
|---|---|
| Pages (from-to) | 385-390 |
| Number of pages | 6 |
| Journal | Astrophysics and Space Science |
| Volume | 23 |
| Issue number | 2 |
| DOIs | |
| State | Published - Aug 1973 |
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