Astronomy and Astrophysics – Astrophysics
Scientific paper
Nov 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998a%26a...339..840s&link_type=abstract
Astronomy and Astrophysics, v.339, p.840-845 (1998)
Astronomy and Astrophysics
Astrophysics
4
Stars: Activity, Stars: Coronae, Stars: Late-Type, Stars: Magnetic Fields, X-Rays: Stars
Scientific paper
The correlation between the coronal X-ray temperature and the magnetic field strength in late-type stars is investigated, based on data primarily from the ROSAT PSPC. According to the observation, we divide the stars into three groups: single, binary and RS CVn stars. From the sample of single stars, we find a clear correlation of the coronal temperature with the magnetic field strength. We interpret that result as the magnetic heating process.
Shi Jian-Rong
You Jun-Han
Zhao Gang
Zhao Yong-Heng
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