088375
收藏DataCite Commons2024-05-16 更新2024-07-13 收录
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http://esdcdoi.esac.esa.int/doi/html/data/astronomy/xmm-newton/088375.html
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We propose to observe the complete sample of confirmed binary Be stars with sdO companions. We aim to probe the essentials of binary evolution theory which predicts that Be-type stars are the products of close binary evolution and that a significant fraction of them have hot companions which were stripped of hydrogen during a mass exchange event. The proposed survey will lead to a characterization of X-ray emission from Be+sdO binaries and establishing their X-ray properties. Furthermore we propose to measure the X-ray spectra of two prototypical Be+sdO systems phi Per and o Pup to measure the hot plasma temperatures and emission measure and to validate a hypothesis about stellar wind collisions in Be binaries. [truncated! Please see actual data for full text]
提供机构:
European Space Agency
创建时间:
2024-05-16



