Here we present a search for new microquasars among the sources detected with the INTEGRAL satellite (IGR sources). We focus on radio emitting IGR sources and report the discovery of two new probable extragalactic sources behind the galactic plane, as well as the detection at higher energies of the ASCA source AX J1639.0-4642, probably a new microquasar in the Galaxy and coincident with a high-energy gamma-ray emitting EGRET source.Fil: Ribó, Marc. CEA Saclay; FranciaFil: Combi, Jorge Ariel. Universidad de Jaén; España. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La ...
Microquasars are stellar x-ray binaries that behave as a scaled down version of extragalactic quasar...
A&A in press, The official date of acceptance is 25/01/2008, 17 pages, 4 figures, 9 tables. New vers...
Invited contribution at "A population explosion: the nature and evolution of X-ray binaries in diver...
The International Gamma-Ray Astrophysics Laboratory (INTEGRAL) is discovering hundreds of new hard X...
Recent studies of relativistic jet sources in the Galaxy, also known as microquasars, have been very...
We present a multiwavelength study of the field containing the unidentified X-ray source AX J1639.0-...
Invited talk to the press conference. 3 pages, 1 figure.International audienceA new type of high-ene...
We present a multiwavelength study of the environment of the unidentified X-ray/ã-ray sources IGR J1...
We report on the identification of a new soft gamma-ray source, IGR J12319 C0749, detected with the ...
International audienceContext: In its first 4 years of observing the sky above 20 keV, INTEGRAL-ISGR...
We report on the identification of a soft gamma-ray source, IGR J172043554, detected with IBIS, the ...
The recent discovery by Paredes et al. (\cite{Paredes}) of a persistent microquasar that is position...
Microquasars are promising candidates to emit high-energy gamma-rays. Moreover, statistical studies ...
We report the discovery of a soft gamma ray source, namely IGR J18135-1751, detected with the IBIS i...
Invited talk at the Frascati Workshop 2007, Vulcano, Italy, May 28 - June 2; Multifrequency Behaviou...
Microquasars are stellar x-ray binaries that behave as a scaled down version of extragalactic quasar...
A&A in press, The official date of acceptance is 25/01/2008, 17 pages, 4 figures, 9 tables. New vers...
Invited contribution at "A population explosion: the nature and evolution of X-ray binaries in diver...
The International Gamma-Ray Astrophysics Laboratory (INTEGRAL) is discovering hundreds of new hard X...
Recent studies of relativistic jet sources in the Galaxy, also known as microquasars, have been very...
We present a multiwavelength study of the field containing the unidentified X-ray source AX J1639.0-...
Invited talk to the press conference. 3 pages, 1 figure.International audienceA new type of high-ene...
We present a multiwavelength study of the environment of the unidentified X-ray/ã-ray sources IGR J1...
We report on the identification of a new soft gamma-ray source, IGR J12319 C0749, detected with the ...
International audienceContext: In its first 4 years of observing the sky above 20 keV, INTEGRAL-ISGR...
We report on the identification of a soft gamma-ray source, IGR J172043554, detected with IBIS, the ...
The recent discovery by Paredes et al. (\cite{Paredes}) of a persistent microquasar that is position...
Microquasars are promising candidates to emit high-energy gamma-rays. Moreover, statistical studies ...
We report the discovery of a soft gamma ray source, namely IGR J18135-1751, detected with the IBIS i...
Invited talk at the Frascati Workshop 2007, Vulcano, Italy, May 28 - June 2; Multifrequency Behaviou...
Microquasars are stellar x-ray binaries that behave as a scaled down version of extragalactic quasar...
A&A in press, The official date of acceptance is 25/01/2008, 17 pages, 4 figures, 9 tables. New vers...
Invited contribution at "A population explosion: the nature and evolution of X-ray binaries in diver...