Optical analysis of an x-ray selected sample of stars.
I analyse an x-ray selected sample of 128 late-type (F-M) stars. 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 stars were reobserved with an extensive pr...
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| Language: | en |
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The University of Arizona.
1988
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| Online Access: | http://hdl.handle.net/10150/184366 |