The cause of intermittent outbursts in radiative hydrodynamic stellar models
The cause of intermittent outbursts found in the pulsations of radiative hydrodynamic stellar models is discussed. The effect of radiation pressure, which will not yield the outbursts in convective models, can be a candidate process for the phenomena. (Author)
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| Published in | Astrophysics and space science Vol. 140; no. 2; pp. 431 - 434 |
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| Main Author | |
| Format | Journal Article |
| Language | English |
| Published |
1988
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| Online Access | Get full text |
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| Summary: | The cause of intermittent outbursts found in the pulsations of radiative hydrodynamic stellar models is discussed. The effect of radiation pressure, which will not yield the outbursts in convective models, can be a candidate process for the phenomena. (Author) |
|---|---|
| Bibliography: | ObjectType-Article-2 SourceType-Scholarly Journals-1 ObjectType-Feature-1 content type line 23 |
| ISSN: | 0004-640X 1572-946X |
| DOI: | 10.1007/BF00638997 |