Accretion Disk Parameters in Cataclysmic Variables

Details Accretion Disk Parameters in Cataclysmic Variables Accretion Disk Parameters in Cataclysmic Variables

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

Affiliated with

Also associated with

No associations

Rating

Accretion Disk Parameters in Cataclysmic Variables does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Accretion Disk Parameters in Cataclysmic Variables, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Accretion Disk Parameters in Cataclysmic Variables will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1706906