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Article: Magnetic Field Structure and Faraday Rotation of the Plerionic Supernova Remnant G21.5–0.9

TitleMagnetic Field Structure and Faraday Rotation of the Plerionic Supernova Remnant G21.5–0.9
Authors
Lai, CWNg, SCYBucciantini, N
Issue Date2022
PublisherIOP Publishing. The Journal's web site is located at http://iopscience.iop.org/0004-637X/
Citation
The Astrophysical Journal, 2022, v. 930 n. 1, p. 1:1-10 How to Cite?
DOI: http://dx.doi.org/10.3847/1538-4357/ac63b1
Persistent Identifierhttp://hdl.handle.net/10722/312902
ISI Accession Number ID
WOS:000788777000001

 

DC FieldValueLanguage
dc.contributor.authorLai, CW-
dc.contributor.authorNg, SCY-
dc.contributor.authorBucciantini, N-
dc.date.accessioned2022-05-21T11:53:15Z-
dc.date.available2022-05-21T11:53:15Z-
dc.date.issued2022-
dc.identifier.citationThe Astrophysical Journal, 2022, v. 930 n. 1, p. 1:1-10-
dc.identifier.urihttp://hdl.handle.net/10722/312902-
dc.languageeng-
dc.publisherIOP Publishing. The Journal's web site is located at http://iopscience.iop.org/0004-637X/-
dc.relation.ispartofThe Astrophysical Journal-
dc.rightsThe Astrophysical Journal. Copyright © IOP Publishing.-
dc.rightsThis is an author-created, un-copyedited version of an article published in [insert name of journal]. IOP Publishing Ltd is not responsible for any errors or omissions in this version of the manuscript or any version derived from it. The Version of Record is available online at http://dx.doi.org/[insert DOI].-
dc.titleMagnetic Field Structure and Faraday Rotation of the Plerionic Supernova Remnant G21.5–0.9-
dc.typeArticle-
dc.identifier.emailLai, CW: pcwlai@hku.hk-
dc.identifier.emailNg, SCY: ncy@astro.physics.hku.hk-
dc.identifier.authorityNg, SCY=rp01706-
dc.identifier.doi10.3847/1538-4357/ac63b1-
dc.identifier.hkuros333109-
dc.identifier.volume930-
dc.identifier.issue1-
dc.identifier.spage1:1-
dc.identifier.epage10-
dc.identifier.isiWOS:000788777000001-

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