The Hyades Star Cluster X-Ray Luminosity Function and its Variation

Details The Hyades Star Cluster X-Ray Luminosity Function and its Variation The Hyades Star Cluster X-Ray Luminosity Function and its Variation

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983nssl.conf..433z&link_type=abstract

The Nearby Stars and the Stellar Luminosity Function, Proceedings of IAU Colloquium No. 76 held 13-16 June 1983 at Wesleyan Univ

Physics

1

Scientific paper

An X-ray survey of the central region of the Hyades cluster with the Einstein satellite has demonstrated that coronal type soft X-ray emission is a common property of the stars in the cluster. Of the 85 stars surveyed, about half have been detected. More than 80% of the F and G dwarfs are X-ray sources. Nineteen of these stars have been monitored both on short and long time scales. The observations may be explained by a large surface coverage of solar type active regions.

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