Probabilistic orbits and dynamical masses of emission-line binaries
Monthly Notices of the Royal Astronomical Society(2021)
摘要
The observed orbits of emission-line stars may be affected by systematics owing to their broad emission lines being formed in complex and extended environments. This is problematic when orbital parameter probability distributions are estimated assuming radial-velocity data are solely comprised of Keplerian motion plus Gaussian white noise, leading to overconfident and inaccurate orbital solutions,...
更多查看译文
关键词
methods: statistical,binaries: spectroscopic,binaries: visual,stars: emission-line, Be,stars: individual: Eta Carinae, GG Carinae, WR, 140, WR 133
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