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

Date

Authors

Hayashi, Sei

Kajino, F

Naito, T

Asahara, A

Bicknell, Geoffrey

Clay, Roger W

Doi, Y

Edwards, P G

Enomoto, R

Gunji, S

Publisher

Elsevier

Abstract

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.

Keywords

Keywords: Accelerated electrons; Binary systems; Close proximity; Compact stars; COMPTON; Compton process; Confidence levels; Gamma rays: observations; Hard x-ray emission; ISM: individual (W50), jets; Lower limits; Nonthermal; Photon spectra; Set constraints; Sour Gamma rays: observations; ISM: individual (W50), jets; Stars: individual (SS433)

URI

http://hdl.handle.net/1885/20995

Collections

ANU Research Publications

Source

Astroparticle Physics

Type

Journal article

DOI

10.1016/j.astropartphys.2009.06.006

Restricted until

2037-12-31

Downloads

File

Description

01_Hayashi_Search_for_VHE_gamma_rays_from_2009.pdf (944.04 KB)

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