The evolving magnetic topology of AB Doradus

Details The evolving magnetic topology of AB Doradus The evolving magnetic topology of AB Doradus

Dec 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aas...19712909h&link_type=abstract

American Astronomical Society, 197th AAS Meeting, #129.09; Bulletin of the American Astronomical Society, Vol. 33, p.713

Astronomy and Astrophysics

Astronomy

Scientific paper

We use a high resolution spectroscopic technique called Zeeman Doppler imaging to obtain magnetic field maps of the surface of AB Doradus, a rapidly rotating K0 dwarf. The magnetic topology of AB Doradus can be explained in terms of a potential field using observations taken over three years. We discuss what the implications are of these potential field maps towards understanding the types of activity cycles operating in young, active late-type stars.

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