Full metadata record
DC Field | Value | Language |
---|---|---|
dc.contributor.author | 김정리 | * |
dc.date.accessioned | 2019-07-29T16:30:49Z | - |
dc.date.available | 2019-07-29T16:30:49Z | - |
dc.date.issued | 2018 | * |
dc.identifier.issn | 1225-4614 | * |
dc.identifier.other | OAK-24292 | * |
dc.identifier.uri | https://dspace.ewha.ac.kr/handle/2015.oak/250261 | - |
dc.description.abstract | The 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.language | English | * |
dc.publisher | KOREAN ASTRONOMICAL SOCIETY | * |
dc.subject | stars: neutron | * |
dc.subject | pulsars: general | * |
dc.subject | Galaxy: center | * |
dc.title | NEUTRON STARS IN THE GALACTIC CENTER | * |
dc.type | Article | * |
dc.relation.issue | 5 | * |
dc.relation.volume | 51 | * |
dc.relation.index | SCIE | * |
dc.relation.index | SCOPUS | * |
dc.relation.index | KCI | * |
dc.relation.startpage | 165 | * |
dc.relation.lastpage | 170 | * |
dc.relation.journaltitle | JOURNAL OF THE KOREAN ASTRONOMICAL SOCIETY | * |
dc.identifier.doi | 10.5303/JKAS.2018.51.5.165 | * |
dc.identifier.wosid | WOS:000455083800004 | * |
dc.author.google | Kim, Chunglee | * |
dc.author.google | Davies, Melvyn B. | * |
dc.contributor.scopusid | 김정리(55153739600) | * |
dc.date.modifydate | 20240304141730 | * |