A new method for estimating frequency-dependent core shifts in active galactic nucleus jets

We discuss the opacity in the core regions of active galactic nuclei observed with Very Long Baseline Interferometry (VLBI), and describe a new method for deriving the frequency-dependent shifts of the VLBI core from the frequency-dependent time lags of flares observed with single-dish observations....

Full description

Bibliographic Details
Main Authors: Kudryavtseva, Nadia, Gabuzda, D., Aller, M., Aller, H.
Format: Journal Article
Published: Wiley-Blackwell Publishing Ltd. 2011
Online Access:http://hdl.handle.net/20.500.11937/49127
_version_ 1848758171342995456
author Kudryavtseva, Nadia
Gabuzda, D.
Aller, M.
Aller, H.
author_facet Kudryavtseva, Nadia
Gabuzda, D.
Aller, M.
Aller, H.
author_sort Kudryavtseva, Nadia
building Curtin Institutional Repository
collection Online Access
description We discuss the opacity in the core regions of active galactic nuclei observed with Very Long Baseline Interferometry (VLBI), and describe a new method for deriving the frequency-dependent shifts of the VLBI core from the frequency-dependent time lags of flares observed with single-dish observations. Application of the method to the core shifts of the quasar 3C 345 shows a very good agreement between the core shifts directly measured from VLBI observations and derived from flares in the total flux density using the proposed method. The frequency-dependent time lags of flares can be used to derive physical parameters of the jets, such as distance from the VLBI core to the base of the jet and the magnetic fields in the core region. Our estimates for 3C 345 indicate core magnetic fields ≃0.1 G and magnetic field at 1 pc ≃ 0.4 G.
first_indexed 2025-11-14T09:39:45Z
format Journal Article
id curtin-20.500.11937-49127
institution Curtin University Malaysia
institution_category Local University
last_indexed 2025-11-14T09:39:45Z
publishDate 2011
publisher Wiley-Blackwell Publishing Ltd.
recordtype eprints
repository_type Digital Repository
spelling curtin-20.500.11937-491272017-09-13T15:38:04Z A new method for estimating frequency-dependent core shifts in active galactic nucleus jets Kudryavtseva, Nadia Gabuzda, D. Aller, M. Aller, H. We discuss the opacity in the core regions of active galactic nuclei observed with Very Long Baseline Interferometry (VLBI), and describe a new method for deriving the frequency-dependent shifts of the VLBI core from the frequency-dependent time lags of flares observed with single-dish observations. Application of the method to the core shifts of the quasar 3C 345 shows a very good agreement between the core shifts directly measured from VLBI observations and derived from flares in the total flux density using the proposed method. The frequency-dependent time lags of flares can be used to derive physical parameters of the jets, such as distance from the VLBI core to the base of the jet and the magnetic fields in the core region. Our estimates for 3C 345 indicate core magnetic fields ≃0.1 G and magnetic field at 1 pc ≃ 0.4 G. 2011 Journal Article http://hdl.handle.net/20.500.11937/49127 10.1111/j.1365-2966.2011.18808.x Wiley-Blackwell Publishing Ltd. unknown
spellingShingle Kudryavtseva, Nadia
Gabuzda, D.
Aller, M.
Aller, H.
A new method for estimating frequency-dependent core shifts in active galactic nucleus jets
title A new method for estimating frequency-dependent core shifts in active galactic nucleus jets
title_full A new method for estimating frequency-dependent core shifts in active galactic nucleus jets
title_fullStr A new method for estimating frequency-dependent core shifts in active galactic nucleus jets
title_full_unstemmed A new method for estimating frequency-dependent core shifts in active galactic nucleus jets
title_short A new method for estimating frequency-dependent core shifts in active galactic nucleus jets
title_sort new method for estimating frequency-dependent core shifts in active galactic nucleus jets
url http://hdl.handle.net/20.500.11937/49127