Emission Line Variability in Accretion Disks

Details Emission Line Variability in Accretion Disks Emission Line Variability in Accretion Disks

Feb 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002noao.prop....3d&link_type=abstract

NOAO Proposal ID #2002A-0003

Computer Science

Scientific paper

Time-resolved spectrophotometric observations of bright, steady state accretion disks in Cataclysmic Variables (CVs) are proposed aiming the study of the fast sthocastic variability of these systems. We plan to investigate the behavior of the recombination line profile and total flux and compare the properties of flickering flares in the lines with the continuum source. The line profile variability will be analyzed in detail using Doppler Imaging techniques with the goal of locate and quantify the source(s) of line flickering in the accretion flow. Dynamical solutions for the binary system will be also obtained.

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