| 書目名稱 | Physical Processes in Red Giants | | 副標(biāo)題 | Proceedings of the S | | 編輯 | Icko Iben,Alvio Renzini | | 視頻video | http://file.papertrans.cn/747/746917/746917.mp4 | | 叢書名稱 | Astrophysics and Space Science Library | | 圖書封面 |  | | 描述 | In recent years, it has become clear that the red-giant phase is one of the most dramatic periods in a star‘s life, when all of its parts become involved in ways that have both direct and indirect observational consequences. This is most particularly true of low- and intermediate- mass stars during the second ascent of the giant branch. Such stars bring to their surfaces products of nucleosynthesis currently taking place in their deep interiors, they pulsate as Mira variables, develop extended outward-flowing atmospheres that may exhibit maser properties, and shed great quantities of matter, sometimes highly processed, into the inter- stellar medium. The manner in which processed matter is brought to the surface is far from being completely explained, and the precise mechanism or mechanisms whereby matter is ejected from the stellar surface (whether by deposition of Alfven waves, radiation pressure on grains, or as a consequence of so- me large scale envelope instability) has yet to be elucidated to every- one‘s satisfaction. The purpose of the second workshop in Astrophysics, organized by the "Advanced School of Astronomy", was to bring together experts on all the physical process | | 出版日期 | Conference proceedings 1981 | | 關(guān)鍵詞 | Bulge; Galaxy; astronomy; stars; stellar | | 版次 | 1 | | doi | https://doi.org/10.1007/978-94-009-8492-9 | | isbn_softcover | 978-94-009-8494-3 | | isbn_ebook | 978-94-009-8492-9Series ISSN 0067-0057 Series E-ISSN 2214-7985 | | issn_series | 0067-0057 | | copyright | D. Reidel Publishing Company, Dordrecht, Holland 1981 |
The information of publication is updating
|
|
|Archiver|手機(jī)版|小黑屋|
派博傳思國際
( 京公網(wǎng)安備110108008328)
GMT+8, 2025-10-14 00:09
發(fā)表于 2025-3-21 18:12:06
