Measuring the Mass Ratios of X-Ray Transients from the Rotational Broadening of the Secondary Star's Spectrum

Robinson E. L.; Bitner M.

Vol. 20 No. 1 (2004), Contributions

Vol. 20 No. 1 (2004)

Contributions

Measuring the Mass Ratios of X-Ray Transients from the Rotational Broadening of the Secondary Star's Spectrum

Robinson E. L.⁺⁻
Bitner M.⁺⁻

Robinson E. L.

Department of Astronomy, University of Texas, 1 University Station, C1400, Austin, TX 78712, USA

Bitner M.

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Keywords

Binaries: Close
Line: Profiles
Stars: Atmospheres

How to Cite

Measuring the Mass Ratios of X-Ray Transients from the Rotational Broadening of the Secondary Star’s Spectrum. (2004). Revista Mexicana De Astrofísica Y Astronomía Serie De Conferencias, 20(1), 207-207. https://astronomia.unam.mx/journals/rmxac/article/view/2004rmxac..20..207r

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Abstract

We describe a new computer program for calculating the spectra of stars that fill their Roche lobes in close binary stars.

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Measuring the Mass Ratios of X-Ray Transients from the Rotational Broadening of the Secondary Star's Spectrum

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