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Mirabel, I.F.; Rodríguez, L.F. "Sources of relativistic jets in the galaxy" (1999) Annual Review of Astronomy and Astrophysics. 37(1):409-443
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Abstract:

Black holes of stellar mass and neutron stars in binary systems are first detected as hard X-ray sources using high-energy space telescopes. Relativistic jets in some of these compact sources are found by means of multiwavelength observations with ground-based telescopes. The X-ray emission probes the inner accretion disk and immediate surroundings of the compact object, whereas the synchrotron emission from the jets is observed in the radio and infrared bands, and in the future could be detected at even shorter wavelengths. Black-hole X-ray binaries with relativistic jets mimic, on a much smaller scale, many of the phenomena seen in quasars and are thus called microquasars. Because of their proximity, their study opens the way for a better understanding of the relativistic jets seen elsewhere in the Universe. From the observation of two-sided moving jets it is inferred that the ejecta in microquasars move with relativistic speeds similar to those believed to be present in quasars. The simultaneous multiwavelength approach to microquasars reveals in short timescales the close connection between instabilities in the accretion disk seen in the X-rays, and the ejection of relativistic clouds of plasma observed as synchrotron emission at longer wavelengths. Besides contributing to a deeper understanding of accretion disks and jets, microquasars may serve in the future to determine the distances of jet sources using constraints from special relativity, and the spin of black holes using general relativity.

Registro:

Documento: Artículo
Título:Sources of relativistic jets in the galaxy
Autor:Mirabel, I.F.; Rodríguez, L.F.
Filiación:Centre d'Etudes de Saclay, CEA/DSM/DAPNIA/Sap, F-91191 Gif-sur-Yvette, France
Inst. Astronomia y Fis. Espacio C., Suc. 28, 1428, Buenos Aires, Argentina
Instituto de Astronomía, UNAM, Apdo. Postal 70-264, 04510 México, D.F, Mexico
Palabras clave:Radio continuum stars; Superluminal motion; X-rays binaries
Año:1999
Volumen:37
Número:1
Página de inicio:409
Página de fin:443
DOI: http://dx.doi.org/10.1146/annurev.astro.37.1.409
Título revista:Annual Review of Astronomy and Astrophysics
Título revista abreviado:Annu. Rev. Astron. Astrophys.
ISSN:00664146
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00664146_v37_n1_p409_Mirabel

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Citas:

---------- APA ----------
Mirabel, I.F. & Rodríguez, L.F. (1999) . Sources of relativistic jets in the galaxy. Annual Review of Astronomy and Astrophysics, 37(1), 409-443.
http://dx.doi.org/10.1146/annurev.astro.37.1.409
---------- CHICAGO ----------
Mirabel, I.F., Rodríguez, L.F. "Sources of relativistic jets in the galaxy" . Annual Review of Astronomy and Astrophysics 37, no. 1 (1999) : 409-443.
http://dx.doi.org/10.1146/annurev.astro.37.1.409
---------- MLA ----------
Mirabel, I.F., Rodríguez, L.F. "Sources of relativistic jets in the galaxy" . Annual Review of Astronomy and Astrophysics, vol. 37, no. 1, 1999, pp. 409-443.
http://dx.doi.org/10.1146/annurev.astro.37.1.409
---------- VANCOUVER ----------
Mirabel, I.F., Rodríguez, L.F. Sources of relativistic jets in the galaxy. Annu. Rev. Astron. Astrophys. 1999;37(1):409-443.
http://dx.doi.org/10.1146/annurev.astro.37.1.409