| 書目名稱 | Variable and Non-spherical Stellar Winds in Luminous Hot Stars |
| 副標(biāo)題 | Proceedings of the I |
| 編輯 | Bernhard Wolf,Otmar Stahl,Alex W. Fullerton |
| 視頻video | http://file.papertrans.cn/981/980525/980525.mp4 |
| 概述 | The IAU-Colloquia are extremely carefully referred and they are used a standard reference for many years.Includes supplementary material: |
| 叢書名稱 | Lecture Notes in Physics |
| 圖書封面 |  |
| 描述 | There is abundant evidence that essentially all luminous hot-star winds contain time-dependent and anisotropic structures. IAU Colloquium 169 was convened to review the observations of variability and asphericity, to discuss the physical processes that might cause such behavior and to look for evolutionary consequences. The topics included OBA stars, Be stars, Wolf-Rayet stars, Be stars, and luminous blue variables (LBVs). The role played by rotation in shaping the stellar wind was a recurrent theme. Photospheric pulsations and/or magnetic fields are particularly appealing mechanisms for triggering the formation of recurrent wind structures. |
| 出版日期 | Conference proceedings 1999 |
| 關(guān)鍵詞 | LOPES; Variation; interferometry; magnetosphere; optical interferometry; spectroscopy; star; star formation |
| 版次 | 1 |
| doi | https://doi.org/10.1007/BFb0106346 |
| isbn_softcover | 978-3-662-14210-3 |
| isbn_ebook | 978-3-540-49062-3Series ISSN 0075-8450 Series E-ISSN 1616-6361 |
| issn_series | 0075-8450 |
| copyright | Springer-Verlag Berlin Heidelberg 1999 |
|Archiver|手機(jī)版|小黑屋|
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