University of Hertfordshire

Time-resolved HST UV echelle spectroscopy of IX Vel

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Documents

  • L.E. Hartley
  • J.E. Drew
  • K.S. Long
View graph of relations
Original languageEnglish
Title of host publicationIn: The Physics of Cataclysmic Variables and Related Objects - ASP Conf Series 261
PublisherAstronomical Society of the Pacific
Pages483-484
ISBN (Print)978-1-58381-597-7, 1-58381-101-X
Publication statusPublished - 2002

Abstract

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.

Notes

Original paper can be found at: http://www.astrosociety.org/pubs/cs/253.html Copyright ASP

ID: 151262