Time-resolved HST UV echelle spectroscopy of IX Vel

Hartley, L.E., Drew, J.E. and Long, K.S. (2002) Time-resolved HST UV echelle spectroscopy of IX Vel. In: In: The Physics of Cataclysmic Variables and Related Objects - ASP Conf Series 261 :. Astronomical Society of the Pacific, pp. 483-484. ISBN 978-1-58381-597-7
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In the hydrodynamical line-driven disk wind models of Proga, Stone & Drew (1998) the mass loss rate is a strong function of the local luminosity. Also, the outflow is found to be subject to clumping, where the main source of driving radiation is the accretion disk. In order to test these predictions, we have obtained high resolution UV spectroscopy of the brightest novalike variable, IX Vel. These data have allowed us to examine the line profile structure in unprecedented detail.
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Additional information Original paper can be found at: http://www.astrosociety.org/pubs/cs/253.html Copyright ASP
Date Deposited 15 May 2025 16:19
Last Modified 15 May 2025 16:19

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