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Intrinsic brightness temperatures of AGN jets

Homan, D. C. and Kovalev, Y. Y. and Lister, M. L. and Ros, E. and Kellermann, K. I. and Cohen, M. H. and Vermeulen, R. C. and Zensus, J. A. and Kadler, M. (2006) Intrinsic brightness temperatures of AGN jets. Astrophysical Journal, 642 (2). L115-L118. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:HOMapjl06

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Abstract

We present a new method for studying the intrinsic brightness temperatures of the parsec-scale jet cores of active galactic nuclei (AGNs). Our method uses observed superluminal motions and observed brightness temperatures for a large sample of AGNs to constrain the characteristic intrinsic brightness temperature of the sample as a whole. To study changes in intrinsic brightness temperature, we assume that the Doppler factors of individual jets are constant in time, as justified by their relatively small changes in observed flux density. We find that in their median-low brightness temperature state, the sources in our sample have a narrow range of intrinsic brightness temperatures centered on a characteristic temperature, Tint_~ 3 × 10 to the 10th K, which is close to the value expected for equipartition, when the energy in the radiating particles equals the energy stored in the magnetic fields. However, in their maximum brightness state, we find that sources in our sample have a characteristic intrinsic brightness temperature greater than 2 × 10 to the 11th K, which is well in excess of the equipartition temperature. In this state, we estimate that the energy in radiating particles exceeds the energy in the magnetic field by a factor of ~ 10 to the 5th. We suggest that the excess of particle energy when sources are in their maximum brightness state is due to injection or acceleration of particles at the base of the jet. Our results suggest that the common method of estimating jet Doppler factors by using a single measurement of observed brightness temperature, the assumption of equipartition, or both may lead to large scatter or systematic errors in the derived values.


Item Type:Article
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URLURL TypeDescription
http://www.journals.uchicago.edu/ApJ/journal/issues/ApJL/v642n2/20400/brief/20400.abstract.htmlOtherUNSPECIFIED
ORCID:
AuthorORCID
Homan, D. C.0000-0002-4431-0890
Kovalev, Y. Y.0000-0001-9303-3263
Lister, M. L.0000-0003-1315-3412
Ros, E.0000-0001-9503-4892
Kellermann, K. I.0000-0002-0093-4917
Additional Information:©2006 The American Astronomical Society. Received 2006 February 3; accepted 2006 March 30; published 2006 April 19. We thank the anonymous referee for helping us to clarify several important points, and A. Lobanov for helpful discussions. This research was supported by an award from Research Corporation and NSF grant AST 04-06923. J.A.Z. acknowledges support from the Max Planck Research Award for International Research Collaboration. M.K. was supported through a stipend from the International Max Planck Research School for Radio and Infrared Astronomy at the University of Bonn.
Subject Keywords:galaxies: active—galaxies: jets—galaxies: kinematics and dynamics—radiation mechanisms: nonthermal—radio continuum: galaxies
Issue or Number:2
Record Number:CaltechAUTHORS:HOMapjl06
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:HOMapjl06
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:5713
Collection:CaltechAUTHORS
Deposited By: Lindsay Cleary
Deposited On:30 Oct 2006
Last Modified:09 Mar 2020 13:19

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