Annual cycles in the interstellar scintillation time-scales of PKSB1519-273 and PKSB1622-253

We have used the University of Tasmania's 30-m radio telescope at Ceduna in South Australia to regularly monitor the flux density of a number of southern blazars. We report the detection of an annual cycle in the variability time-scale of the centimetre radio emission of PKSB1622-253. Observati...

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Main Authors: Carter, S., Ellingsen, S., Macquart, Jean-Pierre, Lovell, J.
Format: Journal Article
Published: Wiley-Blackwell Publishing Ltd. 2009
Subjects:
Online Access:http://hdl.handle.net/20.500.11937/40850
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author Carter, S.
Ellingsen, S.
Macquart, Jean-Pierre
Lovell, J.
author_facet Carter, S.
Ellingsen, S.
Macquart, Jean-Pierre
Lovell, J.
author_sort Carter, S.
building Curtin Institutional Repository
collection Online Access
description We have used the University of Tasmania's 30-m radio telescope at Ceduna in South Australia to regularly monitor the flux density of a number of southern blazars. We report the detection of an annual cycle in the variability time-scale of the centimetre radio emission of PKSB1622-253. Observations of PKS B1519-273 over a period of nearly 2 yr confirm the presence of an annual cycle in the variability time-scale in that source. These observations prove that interstellar scintillation is the principal cause of inter-day variability at radio wavelengths in these sources. The best-fitting annual cycle model for both sources implies a high degree of anisotropy in the scattering screen and that it has a large velocity offset with respect to the local standard of rest. This is consistent with a greater screen distance for these 'slow' intra-day variability(IDV) sources than for rapid scintillators such as PKS B0405-385 or J1819+3845.
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institution Curtin University Malaysia
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publishDate 2009
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spelling curtin-20.500.11937-408502017-09-13T16:05:30Z Annual cycles in the interstellar scintillation time-scales of PKSB1519-273 and PKSB1622-253 Carter, S. Ellingsen, S. Macquart, Jean-Pierre Lovell, J. galaxies active galaxies radio continuum scattering nuclei ISM general We have used the University of Tasmania's 30-m radio telescope at Ceduna in South Australia to regularly monitor the flux density of a number of southern blazars. We report the detection of an annual cycle in the variability time-scale of the centimetre radio emission of PKSB1622-253. Observations of PKS B1519-273 over a period of nearly 2 yr confirm the presence of an annual cycle in the variability time-scale in that source. These observations prove that interstellar scintillation is the principal cause of inter-day variability at radio wavelengths in these sources. The best-fitting annual cycle model for both sources implies a high degree of anisotropy in the scattering screen and that it has a large velocity offset with respect to the local standard of rest. This is consistent with a greater screen distance for these 'slow' intra-day variability(IDV) sources than for rapid scintillators such as PKS B0405-385 or J1819+3845. 2009 Journal Article http://hdl.handle.net/20.500.11937/40850 10.1111/j.1365-2966.2009.14824.x Wiley-Blackwell Publishing Ltd. unknown
spellingShingle galaxies active
galaxies
radio continuum
scattering
nuclei
ISM
general
Carter, S.
Ellingsen, S.
Macquart, Jean-Pierre
Lovell, J.
Annual cycles in the interstellar scintillation time-scales of PKSB1519-273 and PKSB1622-253
title Annual cycles in the interstellar scintillation time-scales of PKSB1519-273 and PKSB1622-253
title_full Annual cycles in the interstellar scintillation time-scales of PKSB1519-273 and PKSB1622-253
title_fullStr Annual cycles in the interstellar scintillation time-scales of PKSB1519-273 and PKSB1622-253
title_full_unstemmed Annual cycles in the interstellar scintillation time-scales of PKSB1519-273 and PKSB1622-253
title_short Annual cycles in the interstellar scintillation time-scales of PKSB1519-273 and PKSB1622-253
title_sort annual cycles in the interstellar scintillation time-scales of pksb1519-273 and pksb1622-253
topic galaxies active
galaxies
radio continuum
scattering
nuclei
ISM
general
url http://hdl.handle.net/20.500.11937/40850