Infrared imaging and polarimetric observations of the pulsar wind nebula in SNR G21.5-0.9-Reference-Cited by-同舟云学术

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Infrared imaging and polarimetric observations of the pulsar wind nebula in SNR G21.5-0.9

Published:2012-05-25 Issue: Volume:542 Page:A12
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Zajczyk A.,Gallant Y. A.,Slane P.,Reynolds S. P.,Bandiera R.,Gouiffès C.,Le Floc’h E.,Comerón F.,Koch Miramond L.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361/201117194/pdf

Reference42 articles.

1. High resolution X-ray and radio images of the Crab-like supernova remnant G21.5-0.9

2. The expansion and radio spectral index of G21.5−0.9: is PSR J1833−1034 the youngest pulsar?

3. The nature of the X-ray halo of the plerion G21.5–0.9 unveiled by XMM-Newton and Chandra

4. Polarization in the inner region of pulsar wind nebulae

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1. IXPE: The Imaging X-ray Polarimetry Explorer;Handbook of X-ray and Gamma-ray Astrophysics;2024

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

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

4. Pulsar Wind Nebulae;Handbook of X-ray and Gamma-ray Astrophysics;2022-11-24

5. Magnetic Field Structure and Faraday Rotation of the Plerionic Supernova Remnant G21.5–0.9;The Astrophysical Journal;2022-04-28

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