抄録
The structure of optically thick mass-losing envelopes of white dwarfs are studied in relation to nova outbursts. A sequence of steady mass-loss solutions is constructed for a nova outburst from the maximum photospheric radius to the disappearance. Much of mass of the envelope will be blown out.
| 本文言語 | English |
|---|---|
| ページ（範囲） | 295-298 |
| ページ数 | 4 |
| ジャーナル | Astrophysics and Space Science |
| 巻 | 99 |
| 号 | 1-2 |
| DOI | |
| 出版ステータス | Published - 1984 2月 1 |
ASJC Scopus subject areas
- 天文学と天体物理学
- 宇宙惑星科学