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Symposium - International Astronomical Union Symposium - International Astronomical Union

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X-ray properties of early-type stars

Published online by Cambridge University Press:  26 May 2016

Thomas W. Berghöfer  and
Jürgen H. M. M. Schmitt
Thomas W. Berghöfer
Affiliation:
Max-Planck-Institut für extraterrestrische Physik Postfach 1603 D-85740 Garching
Jürgen H. M. M. Schmitt
Affiliation:
Max-Planck-Institut für extraterrestrische Physik Postfach 1603 D-85740 Garching
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Extensive stellar surveys with the Einstein Observatory (Chlebowski et al., 1989) and with ROSAT have clearly confirmed the presence of stellar X-ray emission over nearly the whole range of the HR diagram. In the ROSAT all-sky survey data approximately 20000 stellar X-ray sources were detected (Schmitt et al., 1992). Most of these stellar X-ray emitters are low mass late-type stars, the origin of their X-ray emission is thought to be coronal.

Type
3. X-Ray Observations
Information
Symposium - International Astronomical Union , Volume 162: Pulsation, Rotation and Mass Loss in Early-Type Stars , 1994 , pp. 200 - 201
Copyright
Copyright © Kluwer 1994 

References

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