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dc.contributor.authorJones, G.
dc.contributor.authorShannon, Ryan
dc.date.accessioned2017-12-10T12:40:07Z
dc.date.available2017-12-10T12:40:07Z
dc.date.created2017-12-10T12:20:21Z
dc.date.issued2011
dc.identifier.citationJones, G. and Shannon, R. 2011. A joint radio gamma-ray variability study of the crab pulsar, in Torres, D. and Rea, N. (ed), in Proceedings of the First Session of the Sant Cugat Forum on Astrophysics, Apr 12-16 2011, pp. 213-217. Barcelona: Springer-Verlag .
dc.identifier.urihttp://hdl.handle.net/20.500.11937/59380
dc.identifier.doi10.1007/978-3-642-17251-9_17
dc.description.abstract

In order to understand pulsar emission, and coherent emission processes in general, it is important to assess the relationship between high energy and radio emission. Gamma-ray radio correlations can be used to test whether observed radio variability is solely the result of modifications to the radio emission processes (e.g., non-linear wave propagation [1]) or associated with bulk changes in the pulsar magnetosphere and charged particle flow (e.g., [2] and [3]). In the former case, gamma-ray emission would not be correlated with radio variability, but in the latter case, a pronounced correlation between gamma-rays would be expected. Giant radio pulses from the Crab pulsar [4] provide the best opportunity to study this relationship because they occur relatively frequently and provide a non-stationary signal which can be correlated against the high energy emission.

dc.titleA joint radio gamma-ray variability study of the crab pulsar
dc.typeConference Paper
dcterms.source.startPage213
dcterms.source.endPage217
dcterms.source.issn1570-6591
dcterms.source.titleAstrophysics and Space Science Proceedings
dcterms.source.seriesAstrophysics and Space Science Proceedings
curtin.departmentCurtin Institute of Radio Astronomy (Physics)
curtin.accessStatusFulltext not available


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