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Stars at γ-Ray Energies: the INTEGRAL Look at Stars

Published online by Cambridge University Press:  26 May 2016

Thierry Montmerle
Thierry Montmerle*
Affiliation:
Laboratoire d'Astrophysique de Grenoble, France and Service d'Astrophysique, Centre d'Etudes de Saclay, France

Abstract

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The European γ-ray satellite INTEGRAL, launched on October 17, 2002, is the successor to the highly successful American satellite Compton-GRO. Even though its main observational program focuses on “classical” high-energy sources like compact X-ray binaries or AGNs, some time is being devoted to γ-ray studies of massive stars and magnetically active late-type stars. We briefly describe here the four instruments of INTEGRAL, and summarize the ongoing stellar programs.

Type
Part 2: Results from New Instrumentation
Information
Symposium - International Astronomical Union , Volume 219: Stars as Suns : Activity, Evolution and Planets , 2004 , pp. 55 - 62
Copyright
Copyright © Astronomical Society of the Pacific 2004 

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