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A Simple, Unifying Model of the Extreme Ultraviolet Spectra of Dwarf Novae in Outburst

Published online by Cambridge University Press:  22 February 2018

Christopher W. Mauche
Christopher W. Mauche*
Affiliation:
Lawrence Livermore National Laboratory, US

Abstract

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A simple model of the boundary layer and accretion disk wind of dwarf novae in outburst is briefly described and applied to the Chandra Low Energy Transmission Grating spectra of WZ Sge and SS Cyg in outburst.

Resumen

Resumen

Se describe brevemente un modelo simple de la capa limítrofe y del viento del disco de acreción de novas enanas en explosión aplicándolo a los espectros de WZ Sge y SS Cyg en explosión obtenidos con la Rejilla de Transmisión de Baja Energía de Chandra.

Keywords

BinariesClose — NovaeCataclysmic Variables — StarsIndividual (SS CYG, WZ SGE) — StarsWinds, Outflows — UltravioletStars
Type
The Contributed Papers
Information
International Astronomical Union Colloquium , Volume 194: Compact binaries in the galaxy and beyond , 2004 , pp. 174 - 175
Copyright
Copyright © Instituto de astronomia/revista mexicana de astronomίa y astrofίsica 2004

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