CORDIS Project
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This project investigates gamma-ray binaries, which are powerful sources of high-energy radiation in the galaxy. It aims to understand their mechanisms, including particle acceleration and radiation processes, to address unresolved questions in astrophysics.
Gamma-ray binaries are among the most luminous very high-energy sources of the Galaxy.
They consist of a normal star and a compact object, and their radiation is strongly variable and often periodic.
Gamma-ray binaries also generate radio emission of non-thermal and sometimes extended nature, and X-rays, predominantly of non-thermal nature.
These objects are strongly connected with other classes of gamma-ray sources, such as supernova remnants, active galactic nuclei, gamma-ray bursts, and pulsa…
Partner organizations (coordinator is shown above), with normalized type and CORDIS activity type. Guests see up to 4 partners.
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