Interstellar Scintillation and Scattering of Micro-arc-second AGN

The discovery of the first quasar 3C 273 led directly to the discovery of their variability at optical and radio wavelengths. We review the radio variability observations, in particular the variability found at frequencies below 1 GHz, as well as those exhibiting intra-day variability (IDV) at cm wa...

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Main Authors: Jauncey, D., Bignall, H., Kedziora-Chudczer, L., Koay, J., Lovell, J., Macquart, Jean-Pierre, Ojha, R., Pursimo, T., Reynolds, C., Rickett, B.
Format: Journal Article
Published: MDPI AG 2016
Online Access:http://hdl.handle.net/20.500.11937/63057
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author Jauncey, D.
Bignall, H.
Kedziora-Chudczer, L.
Koay, J.
Lovell, J.
Macquart, Jean-Pierre
Ojha, R.
Pursimo, T.
Reynolds, C.
Rickett, B.
author_facet Jauncey, D.
Bignall, H.
Kedziora-Chudczer, L.
Koay, J.
Lovell, J.
Macquart, Jean-Pierre
Ojha, R.
Pursimo, T.
Reynolds, C.
Rickett, B.
author_sort Jauncey, D.
building Curtin Institutional Repository
collection Online Access
description The discovery of the first quasar 3C 273 led directly to the discovery of their variability at optical and radio wavelengths. We review the radio variability observations, in particular the variability found at frequencies below 1 GHz, as well as those exhibiting intra-day variability (IDV) at cm wavelengths. Observations have shown that IDV arises principally from scintillation caused by scattering in the ionized interstellar medium of our Galaxy. The sensitivity of interstellar scintillation towards source angular sizes has provided a powerful tool for studying the most compact components of radio-loud AGN at microarcsecond and milliarcsecond scale resolution.
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institution Curtin University Malaysia
institution_category Local University
last_indexed 2025-11-14T10:24:26Z
publishDate 2016
publisher MDPI AG
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spelling curtin-20.500.11937-630572021-01-13T03:09:38Z Interstellar Scintillation and Scattering of Micro-arc-second AGN Jauncey, D. Bignall, H. Kedziora-Chudczer, L. Koay, J. Lovell, J. Macquart, Jean-Pierre Ojha, R. Pursimo, T. Reynolds, C. Rickett, B. The discovery of the first quasar 3C 273 led directly to the discovery of their variability at optical and radio wavelengths. We review the radio variability observations, in particular the variability found at frequencies below 1 GHz, as well as those exhibiting intra-day variability (IDV) at cm wavelengths. Observations have shown that IDV arises principally from scintillation caused by scattering in the ionized interstellar medium of our Galaxy. The sensitivity of interstellar scintillation towards source angular sizes has provided a powerful tool for studying the most compact components of radio-loud AGN at microarcsecond and milliarcsecond scale resolution. 2016 Journal Article http://hdl.handle.net/20.500.11937/63057 10.3390/galaxies4040062 http://creativecommons.org/licenses/by/4.0/ MDPI AG fulltext
spellingShingle Jauncey, D.
Bignall, H.
Kedziora-Chudczer, L.
Koay, J.
Lovell, J.
Macquart, Jean-Pierre
Ojha, R.
Pursimo, T.
Reynolds, C.
Rickett, B.
Interstellar Scintillation and Scattering of Micro-arc-second AGN
title Interstellar Scintillation and Scattering of Micro-arc-second AGN
title_full Interstellar Scintillation and Scattering of Micro-arc-second AGN
title_fullStr Interstellar Scintillation and Scattering of Micro-arc-second AGN
title_full_unstemmed Interstellar Scintillation and Scattering of Micro-arc-second AGN
title_short Interstellar Scintillation and Scattering of Micro-arc-second AGN
title_sort interstellar scintillation and scattering of micro-arc-second agn
url http://hdl.handle.net/20.500.11937/63057