X-ray irradiation of the winds in binaries with massive components
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361/201525637/pdf
Reference168 articles.
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2. A Steady, Radiative‐Shock Method for Computing X‐Ray Emission from Colliding Stellar Winds in Close, Massive‐Star Binaries
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4. Light Curve Solution of HD 93205 ( \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $\mathrm{O}\,3\mathrm{V}\,+\mathrm{O}\,8\mathrm{V}\,$ \end{document} ) Containing the Earliest Known Star in a Well‐studied Binary
5. Very high energy gamma-rays from Centaurus X-3: Indications and implications
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