Hostname: page-component-848d4c4894-jbqgn Total loading time: 0 Render date: 2024-07-03T07:35:59.873Z Has data issue: false hasContentIssue false

Spectrally Resolved Maps of Optically Thick Accretion Disks

Published online by Cambridge University Press:  12 April 2016

R. Baptista
Affiliation:
Space Telescope Science Institute, USA University of St. Andrews, Scotland, UK
K. Horne
Affiliation:
University of St. Andrews, Scotland, UK
I. Hubeny
Affiliation:
Goddard Space Flight Center, USA
K. Long
Affiliation:
Space Telescope Science Institute, USA
C. W. Mauche
Affiliation:
Lawrence Livermore Nat. Lab., USA
R. G. M. Rutten
Affiliation:
Royal Greenwich Observatory, Tenerife, Canary Islands
R. A. Wade
Affiliation:
Pennsylvania State University, USA

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We report first results of the HST/FOS time-resolved, low-resolution spectroscopy of the eclipsing cataclysmic variable UX UMa, including multi-wavelength mapping of its accretion disk in the ultraviolet region.

Type
Non-Magnetic Cataclysmic Variables
Copyright
Copyright © Kluwer 1996

References

Baptista, R., Steiner, J.E., 1993, A&A, 277, 331 Google Scholar
Horne, K., 1985, MNRAS, 213, 129 Google Scholar