ISSN:
1572-946X
Keywords:
stars: binary
;
stars: individual: Algol, U Sge, U CrB, SW Cyg, RS Vul
Source:
Springer Online Journal Archives 1860-2000
Topics:
Physics
Notes:
Abstract 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.
Type of Medium:
Electronic Resource
URL:
http://dx.doi.org/10.1007/BF00667948
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