Magnetic Fields in Active Late-Type Stars *

Physics

Scientific paper

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Scientific paper

The very high resolution and high signal-to-noise ratio spectra of ten x-ray selected stars are obtained by the NAOC Coudé spectrograph. Magnetic field measurements of these stars have been performed using the profile-addition technique. The magnetic field strength and filling factor are obtained, and we find that there exist strong magnetic fields on very active stars.

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