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eROSITA - Nearby Young Stars in X-rays

Published online by Cambridge University Press:  27 January 2016

J. Robrade
J. Robrade*
Affiliation:
Hamburger Sternwarte, Germany email: jrobrade@hs.uni-hamburg.de
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Abstract

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X-ray surveys are well suited to detect, identify and study young stars based on their high levels of magnetic activity and thus X-ray brightness. The eROSITA instrument onboard the Spectrum-Roentgen-Gamma (SRG) satellite will perform an X-ray all-sky survey that surpasses existing data by a sensitivity increase of more than an order of magnitude. The 4 yr survey is expected to detect more than half a million stars and stellar systems in X-rays.

Keywords

X-rays: starsstars: activitystars: coronae
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Issue S314: Young Stars & Planets Near the Sun , November 2015 , pp. 280 - 285
Copyright
Copyright © International Astronomical Union 2016 

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