Doppler Mapping of SS Cyg: Model vs. Observations

Details Doppler Mapping of SS Cyg: Model vs. Observations Doppler Mapping of SS Cyg: Model vs. Observations

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007jena.confe..93k&link_type=abstract

"JENAM-2007, "Our non-stable Universe", held 20-25 August 2007 in Yerevan, Armenia. Abstract book, p. 93-93"

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Scientific paper

Using the results of 3D gas dynamic simulations of the close binary system SS Cyg synthetic Doppler maps were constructed. The results of computations allowed us to define a shape and location of main gas dynamic features such as disk, stream from inner Lagrangian point, hot line, and spiral waves on the synthetic Doppler maps. The synthetic Doppler maps were compared with observational ones made of three spectral lines H-alpha, H-beta, H-gamma and the main features of the disk structure were identified.

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