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Polarimetric tomography of blazar jets

Published online by Cambridge University Press:  24 March 2015

Ulisses Barres de Almeida ,
Fabrizio Tavecchio  and
Nijil Mankuzhiyil
Ulisses Barres de Almeida
Affiliation:
Centro Brasileiro de Pesquisas Físicas Rua Dr. Xavier Sigaud 150, RJ – 22290-180, Rio de Janeiro, Brazil email: [email protected]
Fabrizio Tavecchio
Affiliation:
Osservatorio Astronomico di Brera, Via Emilio Bianchi 46, 23807 Merate, Italy email: [email protected]
Nijil Mankuzhiyil
Affiliation:
Astrophysics Science Division, BARC, 400085 Mumbai, India email:[email protected]
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Abstract

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In this talk we present a novel way to use optical polarimetric observations to provide independent constraints and guide to the modelling of the spectral energy distribution (SED) of blazars. The approach is particularly useful to judge when a two-zone model description of the SED of the source is required and is able to provide with extra information that helps breaking some of the degeneracies on the fit parameters of the two SSC model components. The method will be presented in some detail and will be subsequently applied to the 2008 multi-wavelength campaign of PKS 2155-304 as an illustration of its potential.

Keywords

polarizationtechniques: polarimetricgalaxies: active
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Issue S313: Extragalactic jets from every angle , September 2014 , pp. 133 - 138
Copyright
Copyright © International Astronomical Union 2015 

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