Progress in the X-ray observation and study of solar like stars.

Details Progress in the X-ray observation and study of solar like stars. Progress in the X-ray observation and study of solar like stars.

Sep 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999pabei..17..244s&link_type=abstract

Prog. Astron., Vol. 17, No. 3, p. 244 - 255

Astronomy and Astrophysics

Astronomy

Solar-Type Stars: X Rays, Solar-Type Stars: Magnetic Fields, Solar-Type Stars: Stellar Coronae, Solar-Type Stars: Stellar Rotation

Scientific paper

The history of researches on the X-ray emission of solar like stars is introduced briefly. With the continuous progress on observational techniques it has been revealed that the magnetic field plays a very important role in the X-ray emission of late-type stars. Here the authors discuss: the corona model where the X-ray is emitted; the dependence of the X-ray emission on the stellar parameters, such as, the rotation or Rossby number, age, spectral type, and the chromospheric activity; the X-ray flare; the long X-ray time variability; the coronal heating mechanisms. Finally, some of research notes for future are briefly discussed.

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