Other
Scientific paper
Jul 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984iue..prop.1767b&link_type=abstract
IUE Proposal ID #CVGWB
Other
Scientific paper
We wish to extend a program begun in Round 6 to study the accretion disk parameters in cataclysmic variables (CVs) with low maw transfer rates. Them are the most common type of CV, but they have been largely ignored by previous IUE observers because they are faint and possess rather cool disks. However, the continuum shapes in these systems are more sensitive to parameters such as the white dwarf maw and Inner and outer disk radii than are the high M systems studied previously. The observed continuum fluxes In the 1200-9000A region will be analyzed by fitting theoretical accretion disks and by applying observational constraints from other wavelength regions
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