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1998A&A...339..840S - Astronomy and Astrophysics, volume 339, 840-845 (1998/11-3)
The relation between the magnetic field strength and the coronal temperature of cool stars.
SHI J.R., ZHAO G., ZHAO Y.-H. and YOU J.-H.
Abstract (from CDS):
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.
Abstract Copyright: ∼
Journal keyword(s): stars: activity - stars: coronae - stars: late-type - stars: magnetic fields - X-rays: stars
Simbad objects: 30
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