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Journal Article
Two Missions, One Microquasar
2009
Overview
The detection of high-energy gamma rays is providing a better picture of the structure and dynamics of microquasars. It has been on the suspect list for more than 30 years, but now we know for sure, smoking gun and all, that x-ray source number 3 in the constellation of Cygnus (Cyg X-3) emits gamma rays. After many near (and wide-of-the-mark) misses, we now have incontrovertible evidence coming from two independent gamma-ray telescopes, AGILE ( 1 ) and Fermi ( 2 ), the latter reported on page 1512 of this issue.
Publisher
American Association for the Advancement of Science,The American Association for the Advancement of Science
Subject
