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Article: Mechanism of the x-ray and soft gamma-ray emissions from high magnetic field pulsar: PSR B1509−58

TitleMechanism of the x-ray and soft gamma-ray emissions from high magnetic field pulsar: PSR B1509−58
Authors
Issue Date2013
PublisherThe American Astronomical Society. The Journal's web site is located at http://iopscience.iop.org/0004-637X/
Citation
The Astrophysical Journal, 2013, v. 764, p. 51:1-16 How to Cite?
Persistent Identifierhttp://hdl.handle.net/10722/181718

 

DC FieldValueLanguage
dc.contributor.authorWang, Yen_US
dc.contributor.authorTakata, Jen_US
dc.contributor.authorCheng, KSen_US
dc.date.accessioned2013-03-19T03:54:40Z-
dc.date.available2013-03-19T03:54:40Z-
dc.date.issued2013en_US
dc.identifier.citationThe Astrophysical Journal, 2013, v. 764, p. 51:1-16en_US
dc.identifier.urihttp://hdl.handle.net/10722/181718-
dc.languageengen_US
dc.publisherThe American Astronomical Society. The Journal's web site is located at http://iopscience.iop.org/0004-637X/en_US
dc.relation.ispartofThe Astrophysical Journalen_US
dc.rightsCreative Commons: Attribution 3.0 Hong Kong License-
dc.titleMechanism of the x-ray and soft gamma-ray emissions from high magnetic field pulsar: PSR B1509−58en_US
dc.typeArticleen_US
dc.identifier.emailTakata, J: takata@hku.hken_US
dc.identifier.emailCheng, KS: hrspksc@hkucc.hku.hken_US
dc.identifier.authorityTakata, J=rp00786en_US
dc.identifier.authorityCheng, KS=rp00675en_US
dc.description.naturepublished_or_final_version-
dc.identifier.doi10.1088/0004-637X/764/1/51-
dc.identifier.hkuros213651en_US
dc.identifier.volume764en_US
dc.identifier.spage51:1en_US
dc.identifier.epage16en_US

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