High-energy emission from jet-clump interactions in microquasars

Astronomy and Astrophysics

Volumn 503, Issue 3, 2009, Pages 673-681

  Araudo, A T ^a,b   Bosch Ramon, V ^c   Romero, G E ^a,b  

^a INSTITUTO ARGENTINO DE RADIOASTRONOMÍA   (Argentina)

^b UNIVERSIDAD NACIONAL DE LA PLATA   (Argentina)

^c MAX PLANCK INSTITUT FÜR KERNPHYSIK   (Germany)

Author keywords

Gamma rays: theory; Radiation mechanisms: non thermal; X rays: binaries

Indexed keywords

BINARY SYSTEMS; COMPACT OBJECTS; DIFFERENT DOMAINS; GAMMA RAYS: THEORY; GAMMA-RAY ASTRONOMY; HIGH ENERGY GAMMA RAYS; HIGH-ENERGY EMISSIONS; HIGH-SENSITIVITY; INVERSE COMPTON; MASSIVE STARS; MICROQUASARS; NEUTRAL PIONS; NON-THERMAL PROCESS; PROTON PROTON COLLISIONS; RADIATION MECHANISMS: NON-THERMAL; RELATIVISTIC JETS; SPECTRAL ENERGY DISTRIBUTION; STELLAR WIND; VERY HIGH ENERGIES; X RAY BINARIES; X-RAYS: BINARIES;

ELECTRIC POWER DISTRIBUTION; HADRONS; HIGH ENERGY PHYSICS; PROTONS; SPECTROSCOPY; STARS; SYNCHROTRONS; SYSTEMS (METALLURGICAL); TELLURIUM COMPOUNDS; WIND POWER; X RAYS;

GAMMA RAYS;

EID: 77950536216     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200811519     Document Type: Article

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