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Synergies in extragalactic and Galactic jet research

Published online by Cambridge University Press:  24 March 2015

Gustavo E. Romero
Gustavo E. Romero*
Affiliation:
Instituto Argentino de Radioastronomía (CCT La Plata, CONICET), C.C.5, (1894) Villa Elisa, Buenos Aires, Argentina email: romero@iar-conicet.gov.ar Facultad de Ciencias Astronómicas y Geofísicas, Universidad Nacional de La Plata, Paseo del Bosque, B1900FWA La Plata, Argentina email: romero@fcaglp.unlp.edu.ar
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Abstract

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The discovery of relativistic jets and superluminal sources associated with accreting X-ray binaries in the Galaxy opened new ways of investigating the physics of outflows from compact objects. The short timescales and relatively large angular sizes of Galactic jets allow to probe the physics of relativistic outflows to unprecedented details. In this article I discuss results of recent modelling of Galactic jets, covering both radiative and dynamical aspects, which can shed light on different features of their extragalactic cousins.

Keywords

jetsmicroquasarsgalaxies: active
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Issue S313: Extragalactic jets from every angle , September 2014 , pp. 361 - 369
Copyright
Copyright © International Astronomical Union 2015 

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