The Effective Temperatures of Hot Stars. II. The Early‐O Types
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/606/i=1/a=497/pdf
Reference107 articles.
1. VLA radio continuum measurements of mass loss from early-type stars
2. The ages and dimensions of Trapezium systems
3. 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
4. Calculation of the masses of the binary star HD 93205 by application of the theory of apsidal motion
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