DC Field | Value | Language |
---|---|---|
dc.contributor.author | Shinn, JH | ko |
dc.contributor.author | Min, KyoungWook | ko |
dc.contributor.author | Lee, CN | ko |
dc.contributor.author | Edelstein, J | ko |
dc.contributor.author | Korpela, EJ | ko |
dc.contributor.author | Welsh, BY | ko |
dc.contributor.author | Han, W | ko |
dc.contributor.author | Nam, UW | ko |
dc.contributor.author | Jin, H | ko |
dc.contributor.author | Lee, DH | ko |
dc.date.accessioned | 2013-03-06T18:03:55Z | - |
dc.date.available | 2013-03-06T18:03:55Z | - |
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.L189 - L192 | - |
dc.identifier.issn | 0004-637X | - |
dc.identifier.uri | http://hdl.handle.net/10203/87880 | - |
dc.description.abstract | Diffuse far-ultraviolet emissions from the Lupus Loop region have been observed with the SPEAR/FIMS instrument. We have detected several important ionic lines, including Si II*, C IV, and N IV], which characterize the warm and hot ionized gas in this region. The spatial variations in the line intensities of Si II* and C IV have also been studied in comparison with X-ray and dust observations. The result shows that they originate from the interface between the hot gas seen in X-rays and the cooler H I shell with which dust is associated. The interface is rather diffuse, and gases with different temperatures seem to coexist in this region. A shock may exist up front in the interface, but its velocity should be very small, as no shock-related distinguishing feature is seen in H alpha. | - |
dc.language | English | - |
dc.publisher | UNIV CHICAGO PRESS | - |
dc.title | Diffuse far-ultraviolet observations of the Lupus Loop region | - |
dc.type | Article | - |
dc.identifier.wosid | 000681634300022 | - |
dc.type.rims | ART | - |
dc.citation.volume | 644 | - |
dc.citation.beginningpage | L189 | - |
dc.citation.endingpage | L192 | - |
dc.citation.publicationname | ASTROPHYSICAL JOURNAL | - |
dc.identifier.doi | 10.1086/505263 | - |
dc.contributor.localauthor | Min, KyoungWook | - |
dc.contributor.nonIdAuthor | Shinn, JH | - |
dc.contributor.nonIdAuthor | Lee, CN | - |
dc.contributor.nonIdAuthor | Edelstein, J | - |
dc.contributor.nonIdAuthor | Korpela, EJ | - |
dc.contributor.nonIdAuthor | Welsh, BY | - |
dc.contributor.nonIdAuthor | Han, W | - |
dc.contributor.nonIdAuthor | Nam, UW | - |
dc.contributor.nonIdAuthor | Jin, H | - |
dc.contributor.nonIdAuthor | Lee, DH | - |
dc.description.isOpenAccess | N | - |
dc.type.journalArticle | Article | - |
dc.subject.keywordAuthor | ISM : bubbles | - |
dc.subject.keywordAuthor | ISM : clouds | - |
dc.subject.keywordAuthor | ISM : evolution | - |
dc.subject.keywordAuthor | ISM : individual (Lupus loop, Lupus cloud) | - |
dc.subject.keywordAuthor | supernova remnants | - |
dc.subject.keywordPlus | SUPER-NOVA REMNANTS | - |
dc.subject.keywordPlus | SCORPIO-CENTAURUS | - |
dc.subject.keywordPlus | H-I | - |
dc.subject.keywordPlus | SN-1006 | - |
dc.subject.keywordPlus | MAPS | - |
dc.subject.keywordPlus | EMISSION | - |
dc.subject.keywordPlus | SPECTRA | - |
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