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Titlebook: Instabilities in Luminous Early Type Stars; Proceedings of a Wor Henny J. G. L. M. Lamers,Camiel W. H. Loore Conference proceedings 1987 D.

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发表于 2025-3-21 18:30:28 | 显示全部楼层 |阅读模式
书目名称Instabilities in Luminous Early Type Stars
副标题Proceedings of a Wor
编辑Henny J. G. L. M. Lamers,Camiel W. H. Loore
视频video
丛书名称Astrophysics and Space Science Library
图书封面Titlebook: Instabilities in Luminous Early Type Stars; Proceedings of a Wor Henny J. G. L. M. Lamers,Camiel W. H. Loore Conference proceedings 1987 D.
描述On April 28 1986 Cornelis de Jager reached the age of 65 years. On April 30 he officially retired from the University of Utrecht where he has held a Chair for Stellar Astrophysics, later changed into Space Physics, since 1958. Cees de Jager, as he prefers to be called by his friends, has had an active and successful life in science. His interest in astronomy was raised by his father under the clear skies of Celebes (Indonesia). He started a study in physics and astronomy as a student of the late M. Minnaert in Utrecht during World War II. When in 1943 the occupying forces recruited students who did not want to sign the declaration of loyalty for their war-efforts, Cees and three fellow students went into hiding at the Observatory in Utrecht. During this very "quiet" period van de Hulst developed the theory of the 21 em radiation of neutral hydrogen and de Jager started the observations of variable stars in the pitch dark nights of a country at war. The study of Beta Cepheids rapid­ ly awoke his interest which was kept throughout the years. In 1958 he organized an international campaign to observe 12 Lac spectroscopically and photometrically, which was a great success.
出版日期Conference proceedings 1987
关键词Galaxy; Variation; galaxies; star; stars; stellar; turbulence
版次1
doihttps://doi.org/10.1007/978-94-009-3901-1
isbn_softcover978-94-010-8232-7
isbn_ebook978-94-009-3901-1Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightD. Reidel Publishing Company, Dordrecht, Holland 1987
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发表于 2025-3-21 20:29:57 | 显示全部楼层
Giant Outbursts of the Eta Carinae - P Cygni TypeDuring such an event, the mass loss rate can be of the order of 0.1 M⨀ yr. for several years. We do not yet understand this phenomenon, partly because most relevant theoretical work has been devoted instead to more familiar, less dramatic stellar winds.
发表于 2025-3-22 02:57:03 | 显示全部楼层
Radiation Driven Instabilitiescur in the supersonic parts of the winds, where as many as one hundred e-folds of linear growth can occur during a typical outflow time. The nonlinear growth of such instabilities can possibly account for the observed superionization and X-ray emission in these stars. Developments in the linear theory of these instabilities is reviewed.
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Non Radially Pulsating Wolf-Rayet Stars initial mass 100 M. losing mass through stellar wind. The periods range from half an hour to a feu hours. The duration of this instability phase is rather short, of the order of a feu e-folding times, uhich are of a feu thousand years.
发表于 2025-3-22 14:53:49 | 显示全部楼层
https://doi.org/10.1007/978-94-009-3901-1Galaxy; Variation; galaxies; star; stars; stellar; turbulence
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Two Comments on the β Cephei Variable 12 LacertaeAccording to a popular notion, the dominant pulsation mode in the g Cephei variables is radial. There is, however, at least one exception to this rule. The exception is 12 Lacertae.
发表于 2025-3-23 06:22:57 | 显示全部楼层
978-94-010-8232-7D. Reidel Publishing Company, Dordrecht, Holland 1987
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