090390
收藏DataCite Commons2024-12-17 更新2025-04-15 收录
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http://esdcdoi.esac.esa.int/doi/html/data/astronomy/xmm-newton/090390.html
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The fate of binary or multiple systems can be violent merger events with massexchange and the ejection of large scale outflows. One of the most recentlydiscovered merger candidates is our target TYC 597-735-1 which harbors a bluering nebular surrounding the rapidly rotating central source. A shortserendipitous Chandra observation suggests three X-ray sources associated withTYC 597-735-1. Here we propose a 50 ks follow-up observation to uncover theorigin of the X-ray emission magnetic activity or shocks as both scenarioshave strong implications for the evolution of stellar merger remnants. [truncated! Please see actual data for full text]
提供机构:
European Space Agency
创建时间:
2024-12-17



