Structure in the radio counterpart to the 2004 December 27 giant flare from SGR 1806-20

Structure in the radio counterpart to the 2004 December 27 giant flare from SGR 1806-20

On 2004 December 27, the magnetar SGR 1806-20 underwent an enormous outburst resulting in the formation of an expanding, moving, and fading radio source. We report observations of this radio source with the Multi-Element Radio-Linked Interferometer Network and the Very Long Baseline Array. The obser...

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Bibliographic Details
Main Authors: Fender, R., Muxlow, T., Garrett, M., Kouveliotou, C., Gaensler, B., Garrington, S., Paragi, Z., Tudose, V., Miller-Jones, James, Spencer, R., Wijers, R., Taylor, G.
Format: Journal Article
Published: Wiley-Blackwell Publishing Ltd. 2006
Subjects:
pulsars: individual: SGR1806-20
radio continuum: stars
ISM: jets and outflows
Online Access:http://onlinelibrary.wiley.com/doi/10.1111/j.1745-3933.2006.00123.x/full
http://hdl.handle.net/20.500.11937/5404

Internet

http://onlinelibrary.wiley.com/doi/10.1111/j.1745-3933.2006.00123.x/full
http://hdl.handle.net/20.500.11937/5404

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