The relation between X-ray emission and rotation in late-type stars from the perspective of X-ray selection

Details The relation between X-ray emission and rotation in late-type stars from the perspective of X-ray selection The relation between X-ray emission and rotation in late-type stars from the perspective of X-ray selection

May 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...340.1011f&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 340, May 15, 1989, p. 1011-1023.

Astronomy and Astrophysics

Astronomy

107

Late Stars, Stellar Rotation, X Ray Sources, Heao 2, Sky Surveys (Astronomy), Stellar Activity, Stellar Coronas

Scientific paper

An X-ray-selected sample of 128 late-type (F-M) stars analyzed. These stars were identified as optical counterparts to serendipitous X-ray detections made by the Einstein Observatory Extended Medium Sensitivity Survey. Once identified as X-ray sources, the sample was followed up by an extensive program of optical observations, including high-resolution and low-resolution spectroscopy and photometry. Spectral types, luminosity classes, distances, X-ray luminosities, projected rotation rates (v sin i), radial velocities, and binary status have been determined for the sample.

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