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Título: | Recollimation shocks in relativistic jets |
Autor: | Martí, José M.; Perucho, Manel; Gómez, José L. CSIC ORCID ; Fuentes, Antonio | Palabras clave: | Galaxies: active Galaxies: jets Magnetohydrodynamics Methods: numerical Shock waves Radiation mechanisms: nonthermal |
Fecha de publicación: | 2018 | Editor: | World Scientific Publishing | Citación: | International Journal of Modern Physics D 27(10): 1844011 (2018) | Resumen: | Recollimation shocks (RS) appear associated with relativistic flows propagating through pressure mismatched atmospheres. Astrophysical scenarios invoking the presence of such shocks include jets from AGNs and X-ray binaries and GRBs. We shall start reviewing the theoretical background behind the structure of RS in overpressured jets. Next, basing on numerical simulations, we will focus on the properties of RS in relativistic steady jets threaded by helical magnetic fields depending on the dominant type of energy. Synthetic radio maps from the simulation of the synchrotron emission for a selection of models in the context of parsec-scale extragalactic jets will also be discussed.© 2018 World Scientific Publishing Company. | Versión del editor: | http://dx.doi.org/10.1142/S021827181844011X | URI: | http://hdl.handle.net/10261/215760 | DOI: | 10.1142/S021827181844011X | Identificadores: | doi: 10.1142/S021827181844011X issn: 0218-2718 |
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