Hostname: page-component-586b7cd67f-dsjbd Total loading time: 0 Render date: 2024-11-25T18:16:21.250Z Has data issue: false hasContentIssue false
  • English
  • Français

Interstellar Scintillation Explains the Intraday Variations in the Linear Polarisation of Quasar PKS 0405-385 at cm-wavelengths

Published online by Cambridge University Press:  05 March 2013

Barney Rickett ,
Lucyna Kedziora-Chudczer  and
David L. Jauncey
Barney Rickett
Affiliation:
University of California San Diego, La Jolla, CA92093, USA; [email protected]
Lucyna Kedziora-Chudczer
Affiliation:
Australia Telescope National Facility and Anglo-Australian Observatory, Sydney, Australia; [email protected]
David L. Jauncey
Affiliation:
Australia Telescope National Facility, Sydney, Australia; [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

During its burst of intraday variation (IDV) in June 1996 quasar PKS 0405–385 exhibited rapid changes in the Stokes parameters Q and U that were even faster than the 1 hr timescale changes in I. Auto- and cross-correlation analyses of I,Q, and U at 8.6 GHz show systematic relations between the variations in I,Q, and U. These are well modelled by interstellar scintillation (ISS) of a 14 × 20 μ as source, with about 180 degree rotation of the polarisation angle along its long dimension. This success in explaining the remarkable IDV in polarisation confirms that ISS gives rise to the IDV in this quasar.

Keywords

galaxies: nucleigalaxies: jetsradio continuum: galaxiesscatteringgalaxies: ISM
Type
Research Article
Information
Publications of the Astronomical Society of Australia , Volume 19 , Issue 1 , 2002 , pp. 106 - 110
Copyright
Copyright © Astronomical Society of Australia 2002

References

Gabuzda, D. C., Kochenov, P., Cawthorne, T. V., & Kollgard, R. 2000a, MNRAS, 313, 627 Google Scholar
Gabuzda, D. C., Kochenov, P., Kollgard, R., & Cawthorne, T. V. 2000b, MNRAS, 315, 229 Google Scholar
Hirabayashi, H., et al. 2000, PASJ, 52, 997 Google Scholar
Kedziora-Chudczer, L., Jauncey, D. L., Wieringa, M. H., Walker, M. A., Nicholson, G. D., Reynolds, J. E., & Tzioumis, A. K. 1997, ApJ, 490, L9 (KC97)CrossRefGoogle Scholar
Kedziora-Chudczer, L., et al. 2001, in Particles and Fields in Radio Galaxies, ASP Conference Series 250, eds R. A. Laing, & K. M. Blundell (San Francisco: ASP)Google Scholar
Little, L. T., & Hewish, A. 1966, MNRAS, 134, 221 Google Scholar
Macquart, J.-P., Kedziora-Chudczer, L., Rayner, D. P., & Jauncey, D. L. 2000, ApJ, 538, 623 Google Scholar
Medvedev, M. 2000, ApJ, 532, L63 CrossRefGoogle Scholar
Qian, S. J., Witzel, A., Kraus, A., Krichbaum, T. P., & Zensus, A. 2001, A&A, 367, 770 Google Scholar
Quirrenbach, A., Witzel, A., Krichbaum, T., Hummel, C. A., Alberdi, A., & Schalinski, C. J. 1989, Nature, 337, 442 Google Scholar
Rickett, B. J. 2001, Ap&SS, 278, 129 Google Scholar
Rickett, B. J. 2002, PASA, 19, 100 Google Scholar
Rickett, B. J., Kedziora-Chudczer, L., & Jauncey, D. L. 2002, ApJ, submittedGoogle Scholar
Rickett, B. J., Quirrenbach, A., Wegner, R., Krichbaum, T., & Witzel, A. 1995, A&A, 293, 479 (R95)Google Scholar