The Radial Velocity and Mass of the White Dwarf of EX Hydrae Measured with Chandra
arXiv:astro-ph/0403665 · doi:10.1086/421389
Abstract
We present the first detection of orbital motion in the cataclysmic variable EX Hydrae based on X-ray data from the Chandra X-ray Observatory. The large collecting area of the telescope and the high resolution of the HETG spectrometers allow for an unprecedented velocity accuracy of ~15 km/s in the X-ray wavelength regime. We find an emission line velocity amplitude of 58.2+-3.7 km/s and infer a white dwarf mass of 0.49+-0.13 M_sun, in good agreement with previous studies using optical, ultraviolet, and far ultraviolet data.
14 pages, 3 figues,accepted for publication by ApJ
References in corpus (5)
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- A precise HST parallax of the cataclysmic variable EX Hydrae, its system parameters, and accretion rate
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