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The winds of cataclysmic variables

Conference ·
OSTI ID:10146833
 [1];  [2]
  1. Lawrence Livermore National Lab., CA (United States). Lab. for Experimental Astrophysics
  2. Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)
The authors present an observational and theoretical review of the winds of cataclysmic variables (CVs). Specifically, they consider the related problems of the geometry and mass-loss rate of the winds of CVs, their ionization state and variability, and the results from studies of eclipsing CVs. Finally, they consider the properties of accretion disk wind models. Some of these models predict substantial angular momentum loss, which could affect both disk structure and binary evolution.
Research Organization:
Lawrence Livermore National Lab., CA (United States)
Sponsoring Organization:
USDOE, Washington, DC (United States); National Aeronautics and Space Administration, Washington, DC (United States)
DOE Contract Number:
W-7405-ENG-48
OSTI ID:
10146833
Report Number(s):
UCRL-JC--116941; CONF-9310316--1; ON: DE94010897; CNN: Grant NAGW-528
Country of Publication:
United States
Language:
English

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