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College of Natural Sciences(자연과학대학)Dept. of Physics(물리학과)PH-Journal Papers(저널논문)

Far-ultraviolet spectral images of the Vela supernova remnant

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dc.contributor.authorNishikida, Kko
dc.contributor.authorEdelstein, Jko
dc.contributor.authorKorpela, EJko
dc.contributor.authorSankrit, Rko
dc.contributor.authorFeuerstein, WMko
dc.contributor.authorMin, KyoungWookko
dc.contributor.authorShinn, JHko
dc.contributor.authorLee, DHko
dc.contributor.authorYuk, ISko
dc.contributor.authorJin, Hko
dc.contributor.authorSeon, KIko
dc.date.accessioned2013-03-06T18:15:24Z-
dc.date.available2013-03-06T18:15:24Z-
dc.date.created2012-02-06-
dc.date.created2012-02-06-
dc.date.created2012-02-06-
dc.date.created2012-02-06-
dc.date.issued2006-06-
dc.identifier.citationASTROPHYSICAL JOURNAL, v.644, pp.L171 - L174-
dc.identifier.issn0004-637X-
dc.identifier.urihttp://hdl.handle.net/10203/87916-
dc.description.abstractWe 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.languageEnglish-
dc.publisherUNIV CHICAGO PRESS-
dc.titleFar-ultraviolet spectral images of the Vela supernova remnant-
dc.typeArticle-
dc.identifier.wosid000681634300018-
dc.type.rimsART-
dc.citation.volume644-
dc.citation.beginningpageL171-
dc.citation.endingpageL174-
dc.citation.publicationnameASTROPHYSICAL JOURNAL-
dc.identifier.doi10.1086/505197-
dc.contributor.localauthorMin, KyoungWook-
dc.contributor.nonIdAuthorNishikida, K-
dc.contributor.nonIdAuthorEdelstein, J-
dc.contributor.nonIdAuthorKorpela, EJ-
dc.contributor.nonIdAuthorSankrit, R-
dc.contributor.nonIdAuthorFeuerstein, WM-
dc.contributor.nonIdAuthorShinn, JH-
dc.contributor.nonIdAuthorLee, DH-
dc.contributor.nonIdAuthorYuk, IS-
dc.contributor.nonIdAuthorJin, H-
dc.contributor.nonIdAuthorSeon, KI-
dc.description.isOpenAccessN-
dc.type.journalArticleArticle-
dc.subject.keywordAuthorISM : individual (Vela supernova remnant)-
dc.subject.keywordAuthorsupernova remnants-
dc.subject.keywordAuthorultraviolet : ISM-
dc.subject.keywordPlusABSORPTION-LINES-
dc.subject.keywordPlusCYGNUS LOOP-
dc.subject.keywordPlusSHOCK-WAVE-
dc.subject.keywordPlusATOMIC DATABASE-
dc.subject.keywordPlusEMISSION-LINES-
dc.subject.keywordPlusHIGH-VELOCITY-
dc.subject.keywordPlusGAS-
dc.subject.keywordPlusSPECTROSCOPY-
dc.subject.keywordPlusCHIANTI-
dc.subject.keywordPlusVI-
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PH-Journal Papers(저널논문)
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