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dc.contributor.author김정리*
dc.date.accessioned2019-07-29T16:30:49Z-
dc.date.available2019-07-29T16:30:49Z-
dc.date.issued2018*
dc.identifier.issn1225-4614*
dc.identifier.otherOAK-24292*
dc.identifier.urihttps://dspace.ewha.ac.kr/handle/2015.oak/250261-
dc.description.abstractThe Galactic Center is one of the most dense stellar environments in the Galaxy and is considered to be a plausible place to harbor many neutron stars. In this brief review, we summarize observational efforts in search of neutron stars within a few degrees about the Galactic Center. Up to 10% of Galactic neutron stars may reside in this central region and it is possible that more than a thousand neutron stars are located within only similar to 25 '' (<= 1 pc) about the Galactic Center. Based on observations, we discuss prospects of detecting neutron stars in the Galactic Center via gravitational waves as well as electromagnetic waves.*
dc.languageEnglish*
dc.publisherKOREAN ASTRONOMICAL SOCIETY*
dc.subjectstars: neutron*
dc.subjectpulsars: general*
dc.subjectGalaxy: center*
dc.titleNEUTRON STARS IN THE GALACTIC CENTER*
dc.typeArticle*
dc.relation.issue5*
dc.relation.volume51*
dc.relation.indexSCIE*
dc.relation.indexSCOPUS*
dc.relation.indexKCI*
dc.relation.startpage165*
dc.relation.lastpage170*
dc.relation.journaltitleJOURNAL OF THE KOREAN ASTRONOMICAL SOCIETY*
dc.identifier.doi10.5303/JKAS.2018.51.5.165*
dc.identifier.wosidWOS:000455083800004*
dc.author.googleKim, Chunglee*
dc.author.googleDavies, Melvyn B.*
dc.contributor.scopusid김정리(55153739600)*
dc.date.modifydate20240304141730*
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자연과학대학 > 물리학전공 > Journal papers
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