Steady mass loss associated with nova outbursts

Mariko Kato

doi:10.1007/BF00650253

Steady mass loss associated with nova outbursts

Mariko Kato

Research output: Contribution to journal › Article › peer-review

Abstract

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.

Original language	English
Pages (from-to)	295-298
Number of pages	4
Journal	Astrophysics and Space Science
Volume	99
Issue number	1-2
DOIs	https://doi.org/10.1007/BF00650253
Publication status	Published - 1984 Feb
Externally published	Yes

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

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10.1007/BF00650253

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title = "Steady mass loss associated with nova outbursts",

abstract = "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.",

author = "Mariko Kato",

year = "1984",

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doi = "10.1007/BF00650253",

language = "English",

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pages = "295--298",

journal = "Astrophysics and Space Science",

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AU - Kato, Mariko

PY - 1984/2

Y1 - 1984/2

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AB - 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.

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JF - Astrophysics and Space Science

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ER -

Steady mass loss associated with nova outbursts

Abstract

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