基本信息
浏览量:245
职业迁徙
个人简介
In collaboration with his former students and colleagues, Dr. Linsky's research involves the analysis of high-resolution stellar spectra, primarily in the ultraviolet, to measure the physical properties of stars, the atmospheres of exoplanets, gas in the local interstellar medium, and the abundance of deuterium in the Galaxy. The primary data set consists of spectra obstained with the COS and STIS instruments on the Hubble Space Telescope (HST), the Far Ultraviolet Spectrograph Explorer (FUSE), and the Chandra X-ray Obseratory (CXO). He and his colleagues have characterized and modelled the chromospheres and higher temperature layers of stars cooler than the Sun including pre-main sequence stars, M dwarf stars, and the host stars of exoplanets. They have developed the astrosphere technique to infer the mass-loss rates of dwarf stars, and have studied accretion phenomena in pre-main sequence stars. Since stellar spectra contain absorption by interstellar gas, they have used such spectra to infer the location, temperature, and kinematics of interstellar gas in partially-ionized interstellar clouds in the solar neighborhood. He has published 582 papers in the refereed astrophysical literature with a citation h index of 75.
研究兴趣
论文共 823 篇作者统计合作学者相似作者
按年份排序按引用量排序主题筛选期刊级别筛选合作者筛选合作机构筛选
时间
引用量
主题
期刊级别
合作者
合作机构
FRONTIERS IN ASTRONOMY AND SPACE SCIENCES (2023)
RAS Techniques and Instrumentsno. 1 (2023): 532-547
引用0浏览0引用
0
0
The Astrophysical Journalno. 2 (2022)
Space Science Reviewsno. 4 (2022): 1-46
arxiv(2022)
加载更多
作者统计
合作学者
合作机构
D-Core
- 合作者
- 学生
- 导师
数据免责声明
页面数据均来自互联网公开来源、合作出版商和通过AI技术自动分析结果,我们不对页面数据的有效性、准确性、正确性、可靠性、完整性和及时性做出任何承诺和保证。若有疑问,可以通过电子邮件方式联系我们:report@aminer.cn