File Download
  Links for fulltext
     (May Require Subscription)
Supplementary

Article: Emission mechanism of GeV-quiet soft gamma-ray pulsars: a case for peculiar geometry?

TitleEmission mechanism of GeV-quiet soft gamma-ray pulsars: a case for peculiar geometry?
Authors
Wang, YNG, CWTakata, JLeung, CKCheng, KS
KeywordsGammarays: stars
Pulsars: general
Radiation mechanisms: non-thermal
Stars: neutron
Issue Date2014
PublisherOxford University press, co-published with Royal Astronomical Society. The Journal's web site is located at http://www.oxfordjournals.org/our_journals/mnras/
Citation
Monthly Notices of the Royal Astronomical Society, 2014, v. 445, p. 604-613 How to Cite?
DOI: http://dx.doi.org/10.1093/mnras/stu1765
Persistent Identifierhttp://hdl.handle.net/10722/207272
ISSN
0035-8711
2021 Impact Factor: 5.235
2020 SCImago Journal Rankings: 2.058
ISI Accession Number ID
WOS:000343827700045

 

DC FieldValueLanguage
dc.contributor.authorWang, Yen_US
dc.contributor.authorNG, CWen_US
dc.contributor.authorTakata, Jen_US
dc.contributor.authorLeung, CKen_US
dc.contributor.authorCheng, KSen_US
dc.date.accessioned2014-12-19T09:57:56Z-
dc.date.available2014-12-19T09:57:56Z-
dc.date.issued2014en_US
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, 2014, v. 445, p. 604-613en_US
dc.identifier.issn0035-8711-
dc.identifier.urihttp://hdl.handle.net/10722/207272-
dc.languageengen_US
dc.publisherOxford University press, co-published with Royal Astronomical Society. The Journal's web site is located at http://www.oxfordjournals.org/our_journals/mnras/en_US
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen_US
dc.rightsThis article has been accepted for publication in Monthly Notices of the Royal Astronomical Society © 2014 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.-
dc.subjectGammarays: stars-
dc.subjectPulsars: general-
dc.subjectRadiation mechanisms: non-thermal-
dc.subjectStars: neutron-
dc.titleEmission mechanism of GeV-quiet soft gamma-ray pulsars: a case for peculiar geometry?en_US
dc.typeArticleen_US
dc.identifier.emailWang, Y: yuwang20@hku.hken_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.doi10.1093/mnras/stu1765en_US
dc.identifier.scopuseid_2-s2.0-84913618516-
dc.identifier.hkuros241735en_US
dc.identifier.volume445en_US
dc.identifier.spage604en_US
dc.identifier.epage613en_US
dc.identifier.isiWOS:000343827700045-
dc.identifier.issnl0035-8711-

Export via OAI-PMH Interface in XML Formats

OR

Export to Other Non-XML Formats