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Keywords

accretion
accretion disks
stars: activity
stars: magnetic field
stars: variables: general

How to Cite

The structure of BB Doradus in quiescence. (2011). Revista Mexicana De Astrofísica Y Astronomía Serie De Conferencias, 40(1), 288-288. https://astronomia.unam.mx/journals/rmxac/article/view/2011rmxac..40..288s
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Abstract

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.