DETECTION OF PERSISTENT GAMMA-RAY EMISSION TOWARD SS433/W50

ABSTRACT The microquasar SS433 features the most energetic jets known in our Galaxy. A large fraction of the jet kinetic power is delivered to the surrounding W50 nebula at the jet termination shock, from which high-energy emission and cosmic-ray production have been anticipated. Here, we report on...

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Veröffentlicht in:	Astrophysical journal. Letters 2015-07, Vol.807 (1), p.L8
Hauptverfasser:	Bordas, P., Yang, R., Kafexhiu, E., Aharonian, F.
Format:	Artikel
Sprache:	eng
Schlagworte:	ASTROPHYSICS, COSMOLOGY AND ASTRONOMY binaries: general COSMIC PROTONS COSMIC RAY FLUX EMISSION ENERGY SPECTRA gamma rays: general GEV RANGE ISM: jets and outflows JETS MEV RANGE MILKY WAY NEBULAE QUASARS STARS stars: individual (SS433) TELESCOPES X-rays: binaries
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