Some Results of Magnetic Field Measurements in Young Stars

Details Some Results of Magnetic Field Measurements in Young Stars Some Results of Magnetic Field Measurements in Young Stars

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007jena.confe..29s&link_type=abstract

"JENAM-2007, "Our non-stable Universe", held 20-25 August 2007 in Yerevan, Armenia. Abstract book, p. 29-29"

Physics

Scientific paper

Results of magnetic field measurements in CTTSs BP Tau and RW Aur are presented. Geometry and time variability of global magnetic field of these stars are discussed. Based on our observations and on the B|| measurements available to date, we argue that, in the case of BP Tau, at least in the He I 5876 line formation region, the magnetic field of the star is not stationary and can be restructured in a time of the order of several hours.

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