Spatially radiative properties of 3C 58 and G21.5−0.9
Author:
Affiliation:
1. Department of Astronomy, Key Laboratory of Astroparticle Physics of Yunnan Province, Yunnan University, Kunming 650091, China
2. Department of Physics, Yuxi Normal University, Yuxi 653100, China
Funder
Natural Science Foundation of China
Natural Science Foundation of Yunnan Province
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/472/3/2926/20131210/stx2223.pdf
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1. THE SECOND FERMI LARGE AREA TELESCOPE CATALOG OF GAMMA-RAY PULSARS
2. CONSTRAINTS ON THE GALACTIC POPULATION OF TeV PULSAR WIND NEBULAE USINGFERMILARGE AREA TELESCOPE OBSERVATIONS
3. THE FIRST FERMI -LAT CATALOG OF SOURCES ABOVE 10 GeV
4. Discovery of TeVγ-ray emission from the pulsar wind nebula 3C 58 by MAGIC
5. HIGH-ENERGY X-RAY IMAGING OF THE PULSAR WIND NEBULA MSH 15–52: CONSTRAINTS ON PARTICLE ACCELERATION AND TRANSPORT
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