Numerical simulation of high Mach number astrophysical jets with radiative cooling

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dc.contributor.authorHa Y.ko
dc.contributor.authorGardner C.L.ko
dc.contributor.authorGelb A.ko
dc.contributor.authorShu C.-W.ko
dc.date.accessioned2013-03-06T07:14:57Z-
dc.date.available2013-03-06T07:14:57Z-
dc.date.created2012-02-06-
dc.date.created2012-02-06-
dc.date.issued2005-
dc.identifier.citationJOURNAL OF SCIENTIFIC COMPUTING, v.24, no.1, pp.597 - 612-
dc.identifier.issn0885-7474-
dc.identifier.urihttp://hdl.handle.net/10203/86241-
dc.description.abstractComputational fluid dynamics simulations using the WENO-LF method are applied to high Mach number nonrelativistic astrophysical jets, including the effects of radiative cooling. Our numerical methods have allowed us to simulate astrophysical jets at much higher Mach numbers than have been attained (Mach 20) in the literature. Our simulations of the HH 1-2 astrophysical jets are at Mach 80. Simulations at high Mach numbers and with radiative cooling are essential for achieving detailed agreement with the astrophysical images.-
dc.languageEnglish-
dc.publisherSPRINGER/PLENUM PUBLISHERS-
dc.subjectESSENTIALLY NONOSCILLATORY SCHEMES-
dc.subjectPROTOSTELLAR JETS-
dc.subjectEFFICIENT IMPLEMENTATION-
dc.subjectSUPERSONIC JETS-
dc.subjectHIGH-ORDER-
dc.subjectSTABILITY-
dc.subjectINSTABILITIES-
dc.subjectINTERFACES-
dc.subjectDYNAMICS-
dc.titleNumerical simulation of high Mach number astrophysical jets with radiative cooling-
dc.typeArticle-
dc.identifier.wosid000230810300002-
dc.identifier.scopusid2-s2.0-23244462525-
dc.type.rimsART-
dc.citation.volume24-
dc.citation.issue1-
dc.citation.beginningpage597-
dc.citation.endingpage612-
dc.citation.publicationnameJOURNAL OF SCIENTIFIC COMPUTING-
dc.identifier.doi10.1007/s10915-004-4786-4-
dc.contributor.nonIdAuthorGardner C.L.-
dc.contributor.nonIdAuthorGelb A.-
dc.contributor.nonIdAuthorShu C.-W.-
dc.type.journalArticleArticle-
dc.subject.keywordAuthorastrophysical jets-
dc.subject.keywordAuthorradiative cooling-
dc.subject.keywordAuthorWENO method-
dc.subject.keywordPlusESSENTIALLY NONOSCILLATORY SCHEMES-
dc.subject.keywordPlusPROTOSTELLAR JETS-
dc.subject.keywordPlusEFFICIENT IMPLEMENTATION-
dc.subject.keywordPlusSUPERSONIC JETS-
dc.subject.keywordPlusHIGH-ORDER-
dc.subject.keywordPlusSTABILITY-
dc.subject.keywordPlusINSTABILITIES-
dc.subject.keywordPlusINTERFACES-
dc.subject.keywordPlusDYNAMICS-
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