A Compact Extreme Scattering Event Cloud toward AO 0235+164

We present observations of a rare, rapid, high-amplitude extreme scattering event toward the compact BL Lac object AO 0235+164 at 6.65 GHz. The ESE cloud is compact; we estimate its diameter between 0.09 and 0.9 AU, with a distance of less than 3.6 kpc. Limits on the angular extent of the ESE cloud...

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Main Authors: Senkbeil, C., Ellingsen, S., Lovell, J., Macquart, Jean-pierre, Cimo, G., Jauncey, D.
Format: Journal Article
Published: The American Astronomical Society 2008
Subjects:
Online Access:http://hdl.handle.net/20.500.11937/25433
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author Senkbeil, C.
Ellingsen, S.
Lovell, J.
Macquart, Jean-pierre
Cimo, G.
Jauncey, D.
author_facet Senkbeil, C.
Ellingsen, S.
Lovell, J.
Macquart, Jean-pierre
Cimo, G.
Jauncey, D.
author_sort Senkbeil, C.
building Curtin Institutional Repository
collection Online Access
description We present observations of a rare, rapid, high-amplitude extreme scattering event toward the compact BL Lac object AO 0235+164 at 6.65 GHz. The ESE cloud is compact; we estimate its diameter between 0.09 and 0.9 AU, with a distance of less than 3.6 kpc. Limits on the angular extent of the ESE cloud imply a minimum cloud electron density of ~4 x 10 3 cm -3. Based on the amplitude and timescale of the ESE observed here, we suggest that at least one of the transients reported by Bower et al. may be attributed to ESEs.
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institution Curtin University Malaysia
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last_indexed 2025-11-14T07:57:00Z
publishDate 2008
publisher The American Astronomical Society
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spelling curtin-20.500.11937-254332023-02-22T06:24:24Z A Compact Extreme Scattering Event Cloud toward AO 0235+164 Senkbeil, C. Ellingsen, S. Lovell, J. Macquart, Jean-pierre Cimo, G. Jauncey, D. individual (AO 0235164) galaxies structure BL Lacertae objects active-ISM We present observations of a rare, rapid, high-amplitude extreme scattering event toward the compact BL Lac object AO 0235+164 at 6.65 GHz. The ESE cloud is compact; we estimate its diameter between 0.09 and 0.9 AU, with a distance of less than 3.6 kpc. Limits on the angular extent of the ESE cloud imply a minimum cloud electron density of ~4 x 10 3 cm -3. Based on the amplitude and timescale of the ESE observed here, we suggest that at least one of the transients reported by Bower et al. may be attributed to ESEs. 2008 Journal Article http://hdl.handle.net/20.500.11937/25433 10.1086/527300 The American Astronomical Society unknown
spellingShingle individual (AO 0235164) galaxies
structure
BL Lacertae objects
active-ISM
Senkbeil, C.
Ellingsen, S.
Lovell, J.
Macquart, Jean-pierre
Cimo, G.
Jauncey, D.
A Compact Extreme Scattering Event Cloud toward AO 0235+164
title A Compact Extreme Scattering Event Cloud toward AO 0235+164
title_full A Compact Extreme Scattering Event Cloud toward AO 0235+164
title_fullStr A Compact Extreme Scattering Event Cloud toward AO 0235+164
title_full_unstemmed A Compact Extreme Scattering Event Cloud toward AO 0235+164
title_short A Compact Extreme Scattering Event Cloud toward AO 0235+164
title_sort compact extreme scattering event cloud toward ao 0235+164
topic individual (AO 0235164) galaxies
structure
BL Lacertae objects
active-ISM
url http://hdl.handle.net/20.500.11937/25433