Doppler Tomography of Accretion Regions in ALGOLS

Details Doppler Tomography of Accretion Regions in ALGOLS Doppler Tomography of Accretion Regions in ALGOLS

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.224..547r&link_type=abstract

Astrophysics and Space Science, Volume 224, Issue 1-2, pp. 547-548

Astronomy and Astrophysics

Astrophysics

2

Stars: Binary, Stars: Individual: Algol, U Sge, U Crb, Sw Cyg, Rs Vul

Scientific paper

The technique of Doppler Tomography has been used to image the accretion regions in five short-period Algols. There is clear evidence of gas flows along the predicted free-fall path of the gas stream as well as asymmetric disk-like structures around the mass gainer. Another source of Hα emission is associated with the cool magnetically active star.

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