Spatially dependent modelling of pulsar wind nebula G0.9+0.1
Author:
Affiliation:
1. Centre for Space Research, North-West University, Potchefstroom Campus, Private Bag X6001, Potchefstroom 2520, South Africa
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/477/3/3853/24813054/sty826.pdf
Reference50 articles.
1. Discovery of gamma-ray emission from the extragalactic pulsar wind nebula N 157B with H.E.S.S.
2. Very high energy gamma rays from the composite SNR G 0.9+0.1
3. THE THEORY OF PULSAR WIND NEBULAE
4. High-resolution radio observations of the supernova remnant G24.7 + 0.6 and the discovery of an ultracompact H II region
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