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Search for VHE gamma rays from SS433/W50 with the CANGAROO-II telescope

Hayashi, Sei; Kajino, F; Naito, T; Asahara, A; Bicknell, Geoffrey; Clay, Roger W; Doi, Y; Edwards, P G; Enomoto, R; Gunji, S; Hara, S; Hara, T; Itoh, Chie

Description

SS433, located at the center of the supernova remnant W50, is a close proximity binary system consisting of a compact star and a normal star. Jets of material are directed outwards from the vicinity of the compact star symmetrically to the east and west.

CollectionsANU Research Publications
Date published: 2009
Type: Journal article
URI: http://hdl.handle.net/1885/20995
Source: Astroparticle Physics
DOI: 10.1016/j.astropartphys.2009.06.006

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