The Radial Velocity and Mass of the White Dwarf of EX Hydrae Measured withChandra
Author(s) -
R. Hoogerwerf,
N. S. Brickhouse,
C. W. Mauche
Publication year - 2004
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/421389
Subject(s) - physics , astrophysics , white dwarf , radial velocity , astronomy , telescope , orbital motion , amplitude , ultraviolet , proper motion , spectrometer , cataclysmic variable star , stars , optics , quantum mechanics , angular momentum
We present the first detection of orbital motion in the cataclysmic variableEX Hydrae based on X-ray data from the Chandra X-ray Observatory. The largecollecting area of the telescope and the high resolution of the HETGspectrometers allow for an unprecedented velocity accuracy of ~15 km/s in theX-ray wavelength regime. We find an emission line velocity amplitude of58.2+-3.7 km/s and infer a white dwarf mass of 0.49+-0.13 M_sun, in goodagreement with previous studies using optical, ultraviolet, and far ultravioletdata.Comment: 14 pages, 3 figues,accepted for publication by Ap
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