Soft X-ray and magnetic field of late-type stars

Details Soft X-ray and magnetic field of late-type stars Soft X-ray and magnetic field of late-type stars

Feb 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998cha%26a..22..479s&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 22, Issue 4, p. 479-486.

Astronomy and Astrophysics

Astrophysics

Scientific paper

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.

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