DC Field | Value | Language |
---|---|---|
dc.contributor.author | Nishikida, K | ko |
dc.contributor.author | Edelstein, J | ko |
dc.contributor.author | Korpela, EJ | ko |
dc.contributor.author | Sankrit, R | ko |
dc.contributor.author | Feuerstein, WM | ko |
dc.contributor.author | Min, KyoungWook | ko |
dc.contributor.author | Shinn, JH | ko |
dc.contributor.author | Lee, DH | ko |
dc.contributor.author | Yuk, IS | ko |
dc.contributor.author | Jin, H | ko |
dc.contributor.author | Seon, KI | ko |
dc.date.accessioned | 2013-03-06T18:15:24Z | - |
dc.date.available | 2013-03-06T18:15:24Z | - |
dc.date.created | 2012-02-06 | - |
dc.date.created | 2012-02-06 | - |
dc.date.created | 2012-02-06 | - |
dc.date.created | 2012-02-06 | - |
dc.date.issued | 2006-06 | - |
dc.identifier.citation | ASTROPHYSICAL JOURNAL, v.644, pp.L171 - L174 | - |
dc.identifier.issn | 0004-637X | - |
dc.identifier.uri | http://hdl.handle.net/10203/87916 | - |
dc.description.abstract | We present far-ultraviolet (FUV) spectral imaging observations of the Vela supernova remnant (SNR) obtained with the SPEAR/FIMS instrument. The Vela SNR extends similar to 8 degrees in the FUV, and its global spectra are dominated by shock-induced emission lines. We find that the global FUV line luminosities can exceed the 0.1 - 2.5 keV soft X-ray luminosity by an order of magnitude. The global O I : C III ratio shows that the Vela SNR has a relatively large fraction of slower shocks compared with the Cygnus Loop. | - |
dc.language | English | - |
dc.publisher | UNIV CHICAGO PRESS | - |
dc.title | Far-ultraviolet spectral images of the Vela supernova remnant | - |
dc.type | Article | - |
dc.identifier.wosid | 000681634300018 | - |
dc.type.rims | ART | - |
dc.citation.volume | 644 | - |
dc.citation.beginningpage | L171 | - |
dc.citation.endingpage | L174 | - |
dc.citation.publicationname | ASTROPHYSICAL JOURNAL | - |
dc.identifier.doi | 10.1086/505197 | - |
dc.contributor.localauthor | Min, KyoungWook | - |
dc.contributor.nonIdAuthor | Nishikida, K | - |
dc.contributor.nonIdAuthor | Edelstein, J | - |
dc.contributor.nonIdAuthor | Korpela, EJ | - |
dc.contributor.nonIdAuthor | Sankrit, R | - |
dc.contributor.nonIdAuthor | Feuerstein, WM | - |
dc.contributor.nonIdAuthor | Shinn, JH | - |
dc.contributor.nonIdAuthor | Lee, DH | - |
dc.contributor.nonIdAuthor | Yuk, IS | - |
dc.contributor.nonIdAuthor | Jin, H | - |
dc.contributor.nonIdAuthor | Seon, KI | - |
dc.description.isOpenAccess | N | - |
dc.type.journalArticle | Article | - |
dc.subject.keywordAuthor | ISM : individual (Vela supernova remnant) | - |
dc.subject.keywordAuthor | supernova remnants | - |
dc.subject.keywordAuthor | ultraviolet : ISM | - |
dc.subject.keywordPlus | ABSORPTION-LINES | - |
dc.subject.keywordPlus | CYGNUS LOOP | - |
dc.subject.keywordPlus | SHOCK-WAVE | - |
dc.subject.keywordPlus | ATOMIC DATABASE | - |
dc.subject.keywordPlus | EMISSION-LINES | - |
dc.subject.keywordPlus | HIGH-VELOCITY | - |
dc.subject.keywordPlus | GAS | - |
dc.subject.keywordPlus | SPECTROSCOPY | - |
dc.subject.keywordPlus | CHIANTI | - |
dc.subject.keywordPlus | VI | - |
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