Circularization in B-type eclipsing binaries in the Magellanic Clouds
暂无分享,去创建一个
[1] M. Marconi,et al. On the Distance of Magellanic Clouds: First Overtone Cepheids , 2002, astro-ph/0206102.
[2] R. E. Wilson,et al. Photometric Solutions for Semidetached Eclipsing Binaries: Selection of Distance Indicators in the Small Magellanic Cloud , 2001, astro-ph/0201255.
[3] R. E. Wilson,et al. Photometric Solutions for Detached Eclipsing Binaries: Selection of Ideal Distance Indicators in the Small Magellanic Cloud , 2001, astro-ph/0105469.
[4] M. Marconi,et al. On the second-overtone stability among Small Magellanic Cloud Cepheids , 2001, astro-ph/0103107.
[5] P. Flower,et al. Transformations from Theoretical Hertzsprung-Russell Diagrams to Color-Magnitude Diagrams: Effective Temperatures, B-V Colors, and Bolometric Corrections , 1996 .
[6] W. Van Hamme,et al. New limb-darkening coefficients for modeling binary star light curves , 1993 .
[7] F. Palla,et al. The pre-main-sequence evolution of intermediate-mass stars , 1993 .
[8] Johannes Andersen,et al. Accurate masses and radii of normal stars , 1991 .
[9] J. Mathis,et al. The relationship between infrared, optical, and ultraviolet extinction , 1989 .
[10] Roger K. Ulrich,et al. Close Binary Stars: Observations and Interpretation , 1980 .
[11] Jacqueline Bergeron,et al. From extrasolar planets to cosmology: the VLT Opening symposium : proceedings of the ESO Symposium held at Antofagasta, Chile, 1-4 March 1999 , 2000 .
[12] Christopher W. Stubbs,et al. The macho project LMC variable star inventory. V. Classification and orbits of 611 eclipsing binary stars , 1997 .
[13] R. E. Wilson,et al. Photometric Solutions for Semi-Detached Eclipsing Binaries : Selection of Distance Indicators in the Small Magellanic Cloud , 2022 .