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Narrow components in UV line profiles as evidence for a two component stellar wind for 0 and B stars

机译：紫外线轮廓中的窄组件作为两个组件恒风的证据为0和B星

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Henny J.G.L.M. Lamers;
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1. Radiation-driven winds of hot luminous stars - XVIII. The unreliability of stellar and wind parameter determinations from optical vs. UV spectral analysis of selected central stars of planetary nebulae and the possibility of some CSPNs as single-star supernova Ia progenitors [J] . T. L. Hoffmann, A. W. A. Pauldrach, C. B. Kaschinski Astronomy and astrophysics . 2016,第21期

机译：发光的恒星的辐射驱动风-XVIII。从选定的行星状星云中央恒星的光学和紫外光谱分析中确定恒星和风参数的可靠性以及某些CSPN作为单星超新星Ia祖先的可能性
2. EVIDENCE FOR DISTINCT COMPONENTS OF THE GALACTIC STELLAR HALO FROM 838 RR LYRAE STARS DISCOVERED IN THE LONEOS-I SURVEY [J] . Antonino Miceli, Armin Rest, Christopher W. Stubbs, The Astrophysical journal . 2008,第2pa1期

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4. O STAR X-RAY LINE PROFILES EXPLAINED BY RADIATION TRANSFER IN INHOMOGENEOUS STELLAR WIND [C] . L. M. Oskinova, A. Feldmeier, W.-R. Hamann Conference on X-ray Universe . 2006

机译：O星X射线线轮廓通过辐射转移在非均匀恒星风中解释
5. Two-Component Galaxies: Understanding the Multiple Stellar Components of Observed and Simulated Galaxies [D] . Lackner, Claire Nicole 2012

机译：两成分星系：了解观测和模拟星系的多个恒星成分
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Narrow components in UV line profiles as evidence for a two component stellar wind for 0 and B stars

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