The structure of BB Doradus in quiescence

Details The structure of BB Doradus in quiescence The structure of BB Doradus in quiescence

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011rmxac..40..288s&link_type=abstract

XIII Latin American Regional IAU Meeting (Eds. W. J. Henney & S. Torres-Peimbert) Revista Mexicana de Astronomía y Astrofísica (

Astronomy and Astrophysics

Astronomy

Accretion, Accretion Disks, Stars: Activity, Stars: Magnetic Field, Stars: Variables: General

Scientific paper

Spectroscopic observations during a low state of BB Dor reveal a complex
emission distribution. Irradiation by the white dwarf as well as
magnetic fields of the secondary star are needed for an explanation.

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