冷恒星的多星系统及其演化
Multiplicity of Cool Stars and their Evolution
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中文总结 AI 辅助
本文总结第23届剑桥冷恒星研讨会分会场关于冷恒星多星性的报告讨论，梳理该领域现状，展望未来，依托近年任务的多星系统研究成果推进冷恒星相关多维度探索。
中文摘要 AI 辅助
多星系统在银河系恒星总数中占相当大的比例，相关研究正迎来复兴。过去十年的任务已发现并表征了大量冷恒星多星系统，这使得研究人员能够探索恒星参数与恒星族群、观测恒星相互作用、研究恒星形成与演化、表征环双星系统，多星系统为冷恒星研究提供了多条研究线索。这一令人兴奋的科学进展只会持续下去，未来的任务将为该主题提供更深入的见解。在本文集中，我们将总结第23届剑桥冷恒星、恒星系统与太阳研讨会上分会场关于冷恒星多星性的报告与讨论，审视该领域的现状并展望未来的发展方向。
英文摘要
Making up a sizeable portion of the galactic census, stellar multiples are experiencing a renaissance. Enabling the study of multiple strands of the study of cool stars, stellar multiples have been found and characterised in great numbers by the missions of the last decade, allowing the exploration of stellar parameters and populations, observation of stellar interactions, studies into stellar formation and evolution, and characterisation of circumbinary systems. This exciting explosion of science is only set to continue, with future missions set to offer even further insights into the topic. Within these proceedings we will summarise the presentations and discussions on cool stellar multiplicity within our splinter sessions at the 23rd Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun, as we examine the present state of the field and look to what the future may bring.
发表机构
- University of Glasgow（格拉斯哥大学）
- KU Leuven（荷语鲁汶大学）
- Chalmers University of Technology（查尔姆斯理工大学）
- Keele University（基尔大学）
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