Steady mass loss associated with nova outbursts

Mariko Kato

研究成果: Article査読

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
99
1-2
DOI
出版ステータスPublished - 1984 2 1

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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