Astrophysics of Single and Binary Star Formation

单星和双星形成的天体物理学

• 批准号: 0205427
• 负责人: Michal Simon
• 金额: $ 26.88万
• 依托单位: SUNY at Stony Brook
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 2002
• 资助国家: 美国
• 起止时间: 2002-07-01 至 2006-06-30
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=0205427&HistoricalAwards=false
• 关键词: Astrophysics; Single; Binary; Star; Formation

AST-0205427PI SimonThis is a program for measuring the masses of pre-main-sequence stars using millimeter wavelength interferometry. Accurate measurements of stellar masses are crucial data, and this work will provide answers to some fundamental astrophysical questions. In particular, it will provide observational constraints on two areas of astrophysical theory that are currently relatively poorly constrained: pre-main-sequence evolutionary tracks, and theories of binary star formation. The PI will also continue his program of the detection of faint secondary companions in single-lined spectroscopic binaries, both to measure the mass ratio distribution of binaries and to provide additional data to use for measuring masses when combined with resolved observations of binary star orbits.

AST-0205427PI模拟这是一个使用毫米波长干涉术测量主序前恒星质量的程序。恒星质量的准确测量是至关重要的数据，这项工作将为一些基本的天体物理问题提供答案。特别是，它将在天体物理理论的两个领域提供观测约束，目前这两个领域的约束相对较差：主序前演化轨迹和双星形成理论。PI还将继续他在单线光谱双星中探测微弱次级伴星的计划，这既是为了测量双星的质量比分布，也是为了提供额外的数据，以便在结合双星轨道的解析观测时用于测量质量。