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  Electromagnetic radiation initiated by hadronic jets from microquasars in the ISM

Bosch-Ramon, V., Aharonian, F., & Paredes, J. M. (2005). Electromagnetic radiation initiated by hadronic jets from microquasars in the ISM. Astronomy & Astrophysics, 432(2), 609-618. doi:10.1051/0004-6361:20041794.

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 Creators:
Bosch-Ramon, Valenti1, Author           
Aharonian, Felix1, Author           
Paredes, J. M.2, Author
Affiliations:
1Division Prof. Dr. Werner Hofmann, MPI for Nuclear Physics, Max Planck Society, ou_904550              
2Departament d'Astronomia i Meteorologia, Universitat de Barcelona, Av. Diagonal 647, 08028 Barcelona, Spain, ou_persistent22              

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Free keywords: X-rays: binaries -- ISM: general -- gamma-rays: observations -- gamma-rays: theory SIMBAD Objects
 Abstract: Microquasars are potential candidates to produce a non-negligible fraction of the observed galactic cosmic rays. The protons accelerated at the jet termination shock interact with the interstellar medium and may produce detectable fluxes of extended emission at different energy bands: high-energy and very high-energy gamma-rays produced by neutral pion-decay, synchrotron and bremsstrahlung emission in a wide energy range generated by the secondary electrons produced by charged pion-decay. We discuss the association between this scenario and some of the unidentified EGRET sources in the galactic plane.

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Language(s): eng - English
 Dates: 2005-03-03
 Publication Status: Issued
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Type: Peer
 Identifiers: eDoc: 276596
DOI: 10.1051/0004-6361:20041794
 Degree: -

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Title: Astronomy & Astrophysics
Source Genre: Journal
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Pages: - Volume / Issue: 432 (2) Sequence Number: - Start / End Page: 609 - 618 Identifier: -