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dc.date.accessioned 2019-10-03T15:25:35Z
dc.date.available 2019-10-03T15:25:35Z
dc.date.issued 2011-02
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/82618
dc.description.abstract Jets are found in a variety of astrophysical sources. In all the cases the jet propagates with a supersonic velocity through the external medium, which can be inhomogeneous, and inhomogeneities could penetrate into the jet. The interaction of the jet material with an obstacle produces a bow-like shock within the jet in which particles can be accelerated up to relativistic energies and emit high-energy photons. In this work, we explore the active galactic nuclei scenario, focusing on the dynamical and radiative consequences of the interaction at different jet heights. We find that the produced high-energy emission could be detectable by the current γ-ray telescopes. In general, the jet-clump interactions are a possible mechanism to produce (steady or flaring) high-energy emission in many astrophysical sources in which jets are present. en
dc.format.extent 131-135 es
dc.language en es
dc.subject Galaxies: active es
dc.subject Radiation mechanisms: nonthermal es
dc.title Radiation from matter entrainment in astrophysical jets: The AGN case en
dc.type Articulo es
sedici.identifier.other http://dx.doi.org/10.1017/s1743921310015802 es
sedici.identifier.issn 1743-9213 es
sedici.creator.person Araudo, Anabella Teresa es
sedici.creator.person Bosch Ramon, V. es
sedici.creator.person Romero, Gustavo Esteban es
sedici.subject.materias Ciencias Astronómicas es
sedici.description.fulltext true es
mods.originInfo.place Facultad de Ciencias Astronómicas y Geofísicas es
sedici.subtype Articulo es
sedici.rights.license Creative Commons Attribution 4.0 International (CC BY 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by/4.0/
sedici.relation.event IAU Symposium 275 (Buenos Aires, Argentina, 13-17 September, 2010) es
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Proceedings of the International Astronomical Union es
sedici.relation.journalVolumeAndIssue vol. 6, no. 275 es


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Creative Commons Attribution 4.0 International (CC BY 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution 4.0 International (CC BY 4.0)