Full metadata record
DC Field | Value | Language |
---|---|---|
dc.contributor.author | 유계화 | - |
dc.date.accessioned | 2016-08-27T02:08:45Z | - |
dc.date.available | 2016-08-27T02:08:45Z | - |
dc.date.issued | 2007 | - |
dc.identifier.issn | 1225-4614 | - |
dc.identifier.other | OAK-4391 | - |
dc.identifier.uri | https://dspace.ewha.ac.kr/handle/2015.oak/216181 | - |
dc.description.abstract | A high resolution spectrum of PU Vul obtained at Bohyunsan Astronomy Observatory on April 9, 2004 is presented. At this phase, PU Vul was an emission-line star and its continuum was very weak. Emission lines of He II, H I, [Ne IV], [N II], [O III], [Ar V] and [Fe VII] dominated the spectrum of PU Vul. Many of them exhibited hat-top profiles with strong and multi-peaked emissions on flat-tops of their profiles. Radial velocities for these lines were measured. Origins of the spectral lines are discussed in terms of the wind and the photoionization models. | - |
dc.language | English | - |
dc.publisher | KOREAN ASTRONOMICAL SOCIETY | - |
dc.subject | symbiotic star : PU Vul | - |
dc.subject | high resolution spectrum : line variations | - |
dc.subject | geometrical structure | - |
dc.title | Nebular spectrum of PU Vul in 2004 | - |
dc.type | Article | - |
dc.relation.issue | 2 | - |
dc.relation.volume | 40 | - |
dc.relation.index | SCIE | - |
dc.relation.index | SCOPUS | - |
dc.relation.index | KCI | - |
dc.relation.startpage | 39 | - |
dc.relation.lastpage | 47 | - |
dc.relation.journaltitle | JOURNAL OF THE KOREAN ASTRONOMICAL SOCIETY | - |
dc.identifier.wosid | WOS:000250779800001 | - |
dc.author.google | Yoo, Kye-Hwa | - |
dc.contributor.scopusid | 유계화(12243560200) | - |
dc.date.modifydate | 20180104081001 | - |