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dc.citation.startPage L14 -
dc.citation.title ASTRONOMY & ASTROPHYSICS -
dc.citation.volume 620 -
dc.contributor.author Lee, Jongsu -
dc.contributor.author Hui, C. Y. -
dc.contributor.author Takata, J. -
dc.contributor.author Lin, L. C. C. -
dc.date.accessioned 2023-12-21T19:48:20Z -
dc.date.available 2023-12-21T19:48:20Z -
dc.date.created 2018-12-31 -
dc.date.issued 2018-12 -
dc.description.abstract We have discovered an extended X-ray feature, apparently associated with millisecond pulsar (MSP) PSR J1911-1114. The feature, which extends for similar to 1', was discovered from an XMM-Newton observation; the radio timing position of PSR J1911-1114 is in the midpoint of the feature. The orientation of the feature is similar to the proper motion direction of PSR J1911-1114. Its X-ray spectrum can be well-modeled by an absorbed power law with a photon index of Gamma = 1.8(-0.2)(+0.3). If this feature is confirmed to be a pulsar wind nebula (PWN), this will be the third case where an X-ray PWN has been found to be powered by a MSP. -
dc.identifier.bibliographicCitation ASTRONOMY & ASTROPHYSICS, v.620, pp.L14 -
dc.identifier.doi 10.1051/0004-6361/201833760 -
dc.identifier.issn 1432-0746 -
dc.identifier.scopusid 2-s2.0-85058860080 -
dc.identifier.uri https://scholarworks.unist.ac.kr/handle/201301/25544 -
dc.identifier.url https://www.aanda.org/articles/aa/abs/2018/12/aa33760-18/aa33760-18.html -
dc.identifier.wosid 000453501400001 -
dc.language 영어 -
dc.publisher EDP SCIENCES S A -
dc.title Discovery of an X-ray nebula in the field of millisecond pulsar PSRJ1911-1114 -
dc.type Article -
dc.description.isOpenAccess FALSE -
dc.relation.journalWebOfScienceCategory Astronomy & Astrophysics -
dc.relation.journalResearchArea Astronomy & Astrophysics -
dc.description.journalRegisteredClass scie -
dc.description.journalRegisteredClass scopus -
dc.subject.keywordAuthor pulsars: individual: PSR J1911-1114 -
dc.subject.keywordAuthor X-rays: stars -
dc.subject.keywordAuthor stars: neutron -

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