Polarimetric Monitoring of Jets with Kanata Telescope

The polarization of relativistic jets is of interest for the understanding of their origin, confinement, and propagation. However, even though numerous measurements have been performed, the mechanisms behind jet variability, creation, and composition are still debated. We have performed simultaneous...

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Main Authors: Ryosuke Itoh, Makoto Uemura, Yasushi Fukazawa, Koji Kawabata
Format: Article
Language:English
Published: MDPI AG 2018-01-01
Series:Galaxies
Subjects:
Online Access:http://www.mdpi.com/2075-4434/6/1/16
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author Ryosuke Itoh
Makoto Uemura
Yasushi Fukazawa
Koji Kawabata
author_facet Ryosuke Itoh
Makoto Uemura
Yasushi Fukazawa
Koji Kawabata
author_sort Ryosuke Itoh
collection DOAJ
description The polarization of relativistic jets is of interest for the understanding of their origin, confinement, and propagation. However, even though numerous measurements have been performed, the mechanisms behind jet variability, creation, and composition are still debated. We have performed simultaneous gamma-ray and optical photopolarimetry observations of 45 blazars with the Kanata telescope since July 2008 to investigate the mechanisms of variability and search for a basic relation between the several subclasses of relativistic jets. Consequently, we found that a correlation between the gamma-ray and optical flux might be related to gamma-ray luminosity, and the maximum polarization degree might be related to gamma-ray luminosity or the ratio of gamma-ray to optical flux. These results imply that low gamma-ray luminosity blazars emit from multiple regions.
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spelling doaj.art-309736bd343d43b1b03ac05746a0e85e2022-12-21T19:28:07ZengMDPI AGGalaxies2075-44342018-01-01611610.3390/galaxies6010016galaxies6010016Polarimetric Monitoring of Jets with Kanata TelescopeRyosuke Itoh0Makoto Uemura1Yasushi Fukazawa2Koji Kawabata3Department of Physics, Tokyo Institute of technology, 2-12-1 Ohokayama, Meguro, Tokyo 152-8551, JapanHiroshima Astrophysical Science Center, Hiroshima University; Higashi-Hiroshima, Hiroshima 739-8526, JapanHiroshima Astrophysical Science Center, Hiroshima University; Higashi-Hiroshima, Hiroshima 739-8526, JapanHiroshima Astrophysical Science Center, Hiroshima University; Higashi-Hiroshima, Hiroshima 739-8526, JapanThe polarization of relativistic jets is of interest for the understanding of their origin, confinement, and propagation. However, even though numerous measurements have been performed, the mechanisms behind jet variability, creation, and composition are still debated. We have performed simultaneous gamma-ray and optical photopolarimetry observations of 45 blazars with the Kanata telescope since July 2008 to investigate the mechanisms of variability and search for a basic relation between the several subclasses of relativistic jets. Consequently, we found that a correlation between the gamma-ray and optical flux might be related to gamma-ray luminosity, and the maximum polarization degree might be related to gamma-ray luminosity or the ratio of gamma-ray to optical flux. These results imply that low gamma-ray luminosity blazars emit from multiple regions.http://www.mdpi.com/2075-4434/6/1/16blazaroptical polarizationgamma-ray
spellingShingle Ryosuke Itoh
Makoto Uemura
Yasushi Fukazawa
Koji Kawabata
Polarimetric Monitoring of Jets with Kanata Telescope
Galaxies
blazar
optical polarization
gamma-ray
title Polarimetric Monitoring of Jets with Kanata Telescope
title_full Polarimetric Monitoring of Jets with Kanata Telescope
title_fullStr Polarimetric Monitoring of Jets with Kanata Telescope
title_full_unstemmed Polarimetric Monitoring of Jets with Kanata Telescope
title_short Polarimetric Monitoring of Jets with Kanata Telescope
title_sort polarimetric monitoring of jets with kanata telescope
topic blazar
optical polarization
gamma-ray
url http://www.mdpi.com/2075-4434/6/1/16
work_keys_str_mv AT ryosukeitoh polarimetricmonitoringofjetswithkanatatelescope
AT makotouemura polarimetricmonitoringofjetswithkanatatelescope
AT yasushifukazawa polarimetricmonitoringofjetswithkanatatelescope
AT kojikawabata polarimetricmonitoringofjetswithkanatatelescope