Abstract： 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.
SHI Jian-Rong;ZHAO Gang;ZHAO Yong-Heng. Magnetic Fields in Active Late-Type Stars[J]. 中国物理快报, 2002, 19(10): 1560-1561.
SHI Jian-Rong, ZHAO Gang, ZHAO Yong-Heng. Magnetic Fields in Active Late-Type Stars. Chin. Phys. Lett., 2002, 19(10): 1560-1561.
2002, Vol. 19 
