RADIO POLARIZATION OBSERVATIONS OF THE SNAIL: A CRUSHED PULSAR WIND NEBULA IN G327.1–1.1 WITH A HIGHLY ORDERED MAGNETIC FIELD-Reference-Cited by-同舟云学术

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RADIO POLARIZATION OBSERVATIONS OF THE SNAIL: A CRUSHED PULSAR WIND NEBULA IN G327.1–1.1 WITH A HIGHLY ORDERED MAGNETIC FIELD

Published:2016-03-24 Issue:2 Volume:820 Page:100
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Ma Y. K.,Ng C.-Y.^ORCID,Bucciantini N.,Slane P. O.^ORCID,Gaensler B. M.^ORCID,Temim T.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/820/i=2/a=100/pdf

Reference40 articles.

1. CONSTRAINTS ON THE GALACTIC POPULATION OF TeV PULSAR WIND NEBULAE USINGFERMILARGE AREA TELESCOPE OBSERVATIONS

2. The magnetic field of the Crab Nebula and the nature of its 'jet'

3. Pulsar Wind Nebulae in Evolved Supernova Remnants

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1. Pulsar Wind Nebulae;Handbook of X-ray and Gamma-ray Astrophysics;2024

2. Radio Study of the Pulsar Wind Nebula Powered by PSR B1706-44;The Astrophysical Journal;2023-03-01

3. Reverberation of pulsar wind nebulae – II. Anatomy of the ‘thin-shell’ evolution;Monthly Notices of the Royal Astronomical Society;2023-01-14

4. The Dawes Review 11: From young to old: The evolutionary path of Pulsar Wind Nebulae;Publications of the Astronomical Society of Australia;2023

5. MeV–GeV Gamma-Ray Emission from SNR G327.1–1.1 Discovered by the Fermi-LAT;The Astrophysical Journal;2022-11-30

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