UNDERSTANDING THE VERY-HIGH-ENERGY EMISSION FROM MICROQUASARS

DOI10.1142/S0218271809014601zbMath1173.85300arXiv0805.4123OpenAlexW2092416717WikidataQ57971296 ScholiaQ57971296MaRDI QIDQ3636382

Valenti Bosch-Ramon, Dmitry Khangulyan

Publication date: 30 June 2009

Published in: International Journal of Modern Physics D (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/0805.4123

zbMATH Keywords

microquasarsoutflowsgamma-ray emissionradiative processes

Mathematics Subject Classification ID

Research exposition (monographs, survey articles) pertaining to relativity and gravitational theory (83-02) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15) Equations of motion in general relativity and gravitational theory (83C10) Astrophysical cosmology (85A40) Statistical astronomy (85A35) Research exposition (monographs, survey articles) pertaining to astronomy and astrophysics (85-02)

Related Items (3)

On a modification of the Rusanov solver for the equations of special relativistic magnetic hydrodynamics ⋮ A new code for the numerical simulation of relativistic flows on supercomputers by means of a low-dissipation scheme ⋮ ELECTRON/POSITRON EXCESSES IN THE COSMIC RAY SPECTRUM AND POSSIBLE INTERPRETATIONS

Cites Work

• Refining the fundamental plane of accreting black holes
• The proton low-mass microquasar: high-energy emission
• Hydromagnetic flows from accretion discs and the production of radio jets
• On the Origin of the Cosmic Radiation

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