Mapping the line emission distribution of cataclysmic variable stars

Details Mapping the line emission distribution of cataclysmic variable stars Mapping the line emission distribution of cataclysmic variable stars

Feb 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.130...85m&link_type=abstract

(IAU, DFG, and Bayerisches Staatsministerium für Unterricht und Kultus, Colloquium on Cataclysmic Variables, Recent Multi-Freque

Astronomy and Astrophysics

Astrophysics

7

Accretion Disks, Cataclysmic Variables, Emission Spectra, Image Reconstruction, Stellar Spectra, Line Spectra, Starspots

Scientific paper

A method for imaging the accretion disc of a cataclysmic variable star
is described. The authors use the two-dimensional information contained
in the line profiles as they vary with phase to invert the line
formation process. Asymmetries in the disc, as are caused by the
bright-spot, for example, are accounted for naturally.

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