A. McNamara, Z. Kuncic, and K. Wu. (2009)cite arxiv:0906.2096
Comment: to appear in "X-ray Polarimetry: A New Window in Astrophysics",
edited by R. Bellazzini, E. Costa, G. Matt and G. Tagliaferri.
Abstract
We investigate the polarization of Compton scattered X-rays from relativistic
jets in active galactic nuclei using Monte Carlo simulations. We consider three
scenarios: scattering of photons from an accretion disk, scattering of cosmic
microwave background (CMB) photons, and synchrotron self-Comptonization (SSC)
within the jet. For Comptonization of thermal disk photons or CMB photons the
maximum linear polarization attained is slightly over 20% at viewing angles
close to 90 degrees. The value decreases with the viewing inclination. For SSC,
the maximum value may exceed 80%. The angle dependence is complicated, and it
varies with the photon injection sites. Our study demonstrates that X-ray
polarization, in addition to multi-wavelength spectra, can distinguish certain
models for emission and particle acceleration in relativistic jets.
cite arxiv:0906.2096
Comment: to appear in "X-ray Polarimetry: A New Window in Astrophysics",
edited by R. Bellazzini, E. Costa, G. Matt and G. Tagliaferri
%0 Journal Article
%1 McNamara2009
%A McNamara, Aimee
%A Kuncic, Zdenka
%A Wu, Kinwah
%D 2009
%K AGN Jets Polarization X-rays
%T Polarization of Compton X-rays from Jets in AGN
%U http://arxiv.org/abs/0906.2096
%X We investigate the polarization of Compton scattered X-rays from relativistic
jets in active galactic nuclei using Monte Carlo simulations. We consider three
scenarios: scattering of photons from an accretion disk, scattering of cosmic
microwave background (CMB) photons, and synchrotron self-Comptonization (SSC)
within the jet. For Comptonization of thermal disk photons or CMB photons the
maximum linear polarization attained is slightly over 20% at viewing angles
close to 90 degrees. The value decreases with the viewing inclination. For SSC,
the maximum value may exceed 80%. The angle dependence is complicated, and it
varies with the photon injection sites. Our study demonstrates that X-ray
polarization, in addition to multi-wavelength spectra, can distinguish certain
models for emission and particle acceleration in relativistic jets.
@article{McNamara2009,
abstract = { We investigate the polarization of Compton scattered X-rays from relativistic
jets in active galactic nuclei using Monte Carlo simulations. We consider three
scenarios: scattering of photons from an accretion disk, scattering of cosmic
microwave background (CMB) photons, and synchrotron self-Comptonization (SSC)
within the jet. For Comptonization of thermal disk photons or CMB photons the
maximum linear polarization attained is slightly over 20% at viewing angles
close to 90 degrees. The value decreases with the viewing inclination. For SSC,
the maximum value may exceed 80%. The angle dependence is complicated, and it
varies with the photon injection sites. Our study demonstrates that X-ray
polarization, in addition to multi-wavelength spectra, can distinguish certain
models for emission and particle acceleration in relativistic jets.
},
added-at = {2009-06-13T02:36:23.000+0200},
author = {McNamara, Aimee and Kuncic, Zdenka and Wu, Kinwah},
biburl = {https://www.bibsonomy.org/bibtex/279ca0693ae367703e723ba10b58ce04c/astravinsky},
description = {Polarization of Compton X-rays from Jets in AGN},
interhash = {04f379a66a024023010aaf492aee41a3},
intrahash = {79ca0693ae367703e723ba10b58ce04c},
keywords = {AGN Jets Polarization X-rays},
note = {cite arxiv:0906.2096
Comment: to appear in "X-ray Polarimetry: A New Window in Astrophysics",
edited by R. Bellazzini, E. Costa, G. Matt and G. Tagliaferri},
timestamp = {2009-06-13T02:36:23.000+0200},
title = {Polarization of Compton X-rays from Jets in AGN},
url = {http://arxiv.org/abs/0906.2096},
year = 2009
}