Hostname: page-component-586b7cd67f-g8jcs Total loading time: 0 Render date: 2024-11-23T14:55:13.724Z Has data issue: false hasContentIssue false

An ESE Event for PSR 0329+54

Published online by Cambridge University Press:  12 April 2016

Anthony Minter*
Affiliation:
National Radio Astronomy Observatory P.O. Box 2, Green Bank, WV, 24944, U.S.A.

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.

Space Very Long Baseline Interferometry observations of PSR 0329+54 which, by luck, occurred during an interstellar fringing event, are presented. Separate images of the pulsar were not detected. However, the pulsar was observed to be extended. The size of PSR 0329+54 during this event is 1.88 × 1.67 mas with a position angle of 30° East of North. This could be due to two separate images of the pulsar separated by ∆θ ≲ 0.5 mas or angular broadening. The observed image size is larger than the expected angular broadening size of < 0.1 mas from the observations of Britton, Gwinn and Ojeda (1998).

Type
Chapter Four Extreme Scattering Events, Distribution of Material and IPS
Copyright
Copyright © Kluwer 2001

References

Britton, M.C., Gwinn, C.R. and Ojeda, M.J.: 1998, Astmphys. J. 501, 101L.CrossRefGoogle Scholar
Clegg, A.W., Fey, A.L. and Lazio, T.J.: 1998, Astmphys. J. 496, 253.CrossRefGoogle Scholar
Hirabayashi, H., Hirosawa, H., Kobayashi, H., et al.: 1998, Science 281, 1825.CrossRefGoogle Scholar
Lazio, T.J.W., Fey, A.L. and Gaume, R.A.: this volume.Google Scholar
Rickett, B.J., Lyne, A.G. and Gupta, Y: 1997, Mon. Not. R. Astron. Soc. 287, 739.CrossRefGoogle Scholar
Taylor, J.H., Manchester, R.N. and Lyne, A.G.: 1993, Astmphys. J. Suppl. 88, 529.CrossRefGoogle Scholar