The deepest radio study of the pulsar wind nebula G21.5−0.9: still no evidence for the supernova shell
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/412/2/1221/5739018/mnras0412-1221.pdf
Reference40 articles.
1. A statistical approach to radio emission from shell-type SNRs
2. High-resolution radio observations of three supernova remnants
3. High resolution X-ray and radio images of the Crab-like supernova remnant G21.5-0.9
4. GLIMPSE. I. AnSIRTFLegacy Project to Map the Inner Galaxy
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