书目名称 | Observational Imprints of Binary Evolution on B- and Be-star Populations | 编辑 | Julia Bodensteiner | 视频video | | 概述 | Establishes a new class of post-interaction binaries briefly after mass transfer.Provides new evidence that a majority of the massive classical Be stars result from binary interactions.Presents a comp | 丛书名称 | Springer Theses | 图书封面 |  | 描述 | This book presents novel observational evidence toward detecting and characterizing the products of massive, interacting binary stars. As a majority of massive stars are born in close binary systems, a large number of so-called massive binary interaction products are predicted to exist; however, few have been identified so far. Based on observations with the largest telescopes around the world, equipped with state-of-the-art instrumentation, this book helps to remedy this situation. In her outstanding PhD-thesis Julia Bodensteiner identifies a new class of post-interaction binaries in a short-lived phase just briefly after the initially more massive star has been stripped of part of its envelope. She further provides new evidence for the Be phenomenon to largely result from binary interactions. These results represented a new and testable prediction for the evolution of these stars and opened up a new way forward for identifying hundreds of post-interaction products..Finally,using the MUSE integral field spectrograph at the Very Large Telescope in Chile, the author presents a novel spectroscopic campaign focusing on the 40 Myr-old star cluster NGC 330 in the Small Magellanic Clouds | 出版日期 | Book 2022 | 关键词 | Binary Evolution; Binary Stars; Massive Stars; Binary Interaction Products; Optical Spectroscopy; Star Cl | 版次 | 1 | doi | https://doi.org/10.1007/978-3-031-19489-4 | isbn_softcover | 978-3-031-19491-7 | isbn_ebook | 978-3-031-19489-4Series ISSN 2190-5053 Series E-ISSN 2190-5061 | issn_series | 2190-5053 | copyright | The Editor(s) (if applicable) and The Author(s), under exclusive license to Springer Nature Switzerl |
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