Emergence and disappearance of microarcsecond structure in the scintillating quasar J1819+3845

The 4.8-GHz light curves of the scintillating intraday variable quasar J1819+3845 during 2004-2005 exhibit sharp structure, down to a time-scale of 15 min, that was absent from lightcurves taken prior to this period and from the 2006 light curves. Analysis of the light curve powerspectra show that t...

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Main Authors: Macquart, Jean-pierre, de Bruyn, A.
Format: Journal Article
Published: Wiley-Blackwell Publishing Ltd. 2007
Subjects:
Online Access:http://hdl.handle.net/20.500.11937/41593
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author Macquart, Jean-pierre
de Bruyn, A.
author_facet Macquart, Jean-pierre
de Bruyn, A.
author_sort Macquart, Jean-pierre
building Curtin Institutional Repository
collection Online Access
description The 4.8-GHz light curves of the scintillating intraday variable quasar J1819+3845 during 2004-2005 exhibit sharp structure, down to a time-scale of 15 min, that was absent from lightcurves taken prior to this period and from the 2006 light curves. Analysis of the light curve powerspectra show that the variations must be due to the emergence of new structure in the source.The power spectra yield a scattering screen distance of 3.8 0.3 pc for a best-fitting vISS = 59 0.5 km s-1 or 2.0 0.3 pc for the scintillation velocity reported by Dennett-Thorpe & de Bruyn. The scattering medium is required to be exceptionally turbulent, with C2N 0.7L-1 pc m-20/3 for scattering material of thickness Lpc pc along the ray path. The 2004 power spectrum can be explained in terms of a double source with a component separation 240 15 as in 2004.
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spelling curtin-20.500.11937-415932017-09-13T16:05:06Z Emergence and disappearance of microarcsecond structure in the scintillating quasar J1819+3845 Macquart, Jean-pierre de Bruyn, A. quasars galaxies individual high angular resolution scattering active techniques J1819+3845 The 4.8-GHz light curves of the scintillating intraday variable quasar J1819+3845 during 2004-2005 exhibit sharp structure, down to a time-scale of 15 min, that was absent from lightcurves taken prior to this period and from the 2006 light curves. Analysis of the light curve powerspectra show that the variations must be due to the emergence of new structure in the source.The power spectra yield a scattering screen distance of 3.8 0.3 pc for a best-fitting vISS = 59 0.5 km s-1 or 2.0 0.3 pc for the scintillation velocity reported by Dennett-Thorpe & de Bruyn. The scattering medium is required to be exceptionally turbulent, with C2N 0.7L-1 pc m-20/3 for scattering material of thickness Lpc pc along the ray path. The 2004 power spectrum can be explained in terms of a double source with a component separation 240 15 as in 2004. 2007 Journal Article http://hdl.handle.net/20.500.11937/41593 10.1111/j.1745-3933.2007.00341.x Wiley-Blackwell Publishing Ltd. unknown
spellingShingle quasars
galaxies
individual
high angular resolution
scattering
active
techniques
J1819+3845
Macquart, Jean-pierre
de Bruyn, A.
Emergence and disappearance of microarcsecond structure in the scintillating quasar J1819+3845
title Emergence and disappearance of microarcsecond structure in the scintillating quasar J1819+3845
title_full Emergence and disappearance of microarcsecond structure in the scintillating quasar J1819+3845
title_fullStr Emergence and disappearance of microarcsecond structure in the scintillating quasar J1819+3845
title_full_unstemmed Emergence and disappearance of microarcsecond structure in the scintillating quasar J1819+3845
title_short Emergence and disappearance of microarcsecond structure in the scintillating quasar J1819+3845
title_sort emergence and disappearance of microarcsecond structure in the scintillating quasar j1819+3845
topic quasars
galaxies
individual
high angular resolution
scattering
active
techniques
J1819+3845
url http://hdl.handle.net/20.500.11937/41593