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Soft X-ray and magnetic field of late-type stars
Authors:Jian-rong Shi  Gang Zhao  Yong-heng Zhao  Jun-han You
Institution:

a Department of Applied Physics, Shanghai Jiaotong University, Shanghai 200240, China

b Beijing Astronomical Observatory, Chinese Academy of Sciences, Beijing 100080, China

Abstract:We used four coronal models to fit ROSAT data of a sample of late-type stars. The merits and demerits of each was discussed. We found a good correlation between the cornoal temperature so derived and the magnetic field strength. This indicates magnetic heating of the corona and provides a possible, indirect means of estimating the photospheric magnetic field.
Keywords:late-type star  X-ray  star corona  magnetic field
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