Coronal soft X-ray emission and the magnetic fields of cool stars.

Details Coronal soft X-ray emission and the magnetic fields of cool stars. Coronal soft X-ray emission and the magnetic fields of cool stars.

Jul 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998acaps..18..293s&link_type=abstract

Acta Astrophys. Sin., Vol. 18, No. 3, p. 293 - 301

Astronomy and Astrophysics

Astrophysics

Late-Type Stars: Magnetic Fields, Late-Type Stars: Stellar Coronae, Late-Type Stars: X Rays, Stellar Coronae: Models

Scientific paper

The correlation between the X-ray emission and the magnetic field in late-type stars is investigated, based on data primarily from the ROSAT PSPC observation. Four coronal models have been considered to fit the sample stars. A strong correlation between the coronal temperature and the magnetic field in single cool stars is found. The authors interpret the result as a magnetic heating process.

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