The CHARA Array resolves the long-period Wolf–Rayet binaries WR 137 and WR 138

Monthly Notices of the Royal Astronomical Society(2016)

引用 13|浏览9
暂无评分
摘要
We report on interferometric observations with the CHARA Array of two classical Wolf–Rayet (WR) stars in suspected binary systems, namely WR 137 and WR 138. In both cases, we resolve the component stars to be separated by a few milliarcseconds. The data were collected in the H band, and provide a measure of the fractional flux for both stars in each system. We find that the WR star is the dominant...
更多
查看译文
关键词
binaries: visual,stars: individual: WR 137,stars: individual: WR 138,stars: mass-loss,stars: winds, outflows,stars: Wolf–Rayet
AI 理解论文
溯源树
样例
生成溯源树,研究论文发展脉络
Chat Paper
正在生成论文摘要