U.S.-U.K. Cooperative Research: Spectroscopy of Faint Cataclysmic Variables

美英合作研究：微弱灾难变量的光谱学

• 批准号: 9014168
• 负责人: Steven Howell
• 金额: $ 1.45万
• 依托单位: Leidos, Inc.
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 1990
• 资助国家: 美国
• 起止时间: 1990-12-01 至 1994-05-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=9014168&HistoricalAwards=false
• 关键词: U.S.; U.K.; Cooperative; Research; Spectroscopy

This award will support collaborative research in astronomy between Dr. Steven Howell, Planetary Science Institute, Tucson, Arizona and Dr. Keith Mason, Mullard Space Science Laboratory, University College London. The objective of the proposed project is to investigate a previously unstudied group of cataclysmic variable stars which may be members of the Galactic halo. The standard picture of a cataclysmic variable (CV) is a close binary system consisting of a late type main sequence star which transfers mass to a white dwarf companion. The material that leaves the secondary forms a disk around the primary star. The intersection of this stream and the disk gives rise to a "hot spot", which can provide a large fraction of the system light. If the white dwarf has a sufficiently strong magnetic field, the transferred material will be disturbed and even the formation of the disk can be retarded. The only direct method of finding the true location of these cataclysmic variables is through distance determination. The investigators are analyzing spectroscopic data, using software which they developed jointly at the Mullard Space Science Laboratory, to model and deconvolve the contributions to the data from the various systems components. This procedure will allow them to derive a distance for these stars. If these binary systems are really located in the Galactic halo, they should have very different properties from their well studied counterparts located in the disk. The results of this study will make an important contribution to understanding the true nature of cataclysmic variables and how these populations differ, as well as to understanding the structure and evolution of our Galaxy in general. The project will benefit from the complementary expertise of the two investigators in the area of theoretical interpretations of binary stars.

该奖项将支持亚利桑那州图森市行星科学研究所的Steven Howell博士和伦敦大学学院Mullard空间科学实验室的Keith Mason博士在天文学方面的合作研究。拟议项目的目标是调查一组以前未被研究过的激变变星，它们可能是银河晕的成员。激变变星(CV)的标准图像是一个紧密的双星系统，它由一颗晚期主序星组成，它将质量转移到白矮星伴星上。离开主星的物质在主星周围形成了一个圆盘。这股光线和圆盘的交叉点形成了一个“热点”，可以提供很大一部分系统光。如果白矮星有足够强的磁场，传送的物质将受到干扰，甚至可以延缓圆盘的形成。找到这些激变变数的真实位置的唯一直接方法是通过距离测定。研究人员正在使用他们在穆拉德空间科学实验室共同开发的软件来分析光谱数据，以对各种系统组件对数据的贡献进行建模和去卷积。这一过程将允许他们推导出这些恒星的距离。如果这些双星系统真的位于银河晕中，它们的性质应该与盘中经过充分研究的对应系统有很大的不同。这项研究的结果将对理解激变变星的真实性质以及这些变星群体的不同之处，以及理解我们银河系的总体结构和演化做出重要贡献。该项目将受益于两位研究人员在双星理论解释领域的互补专业知识。