Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/26084
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dc.contributor.authorDehnen, W-
dc.contributor.authorOdenkirchen, M-
dc.contributor.authorGrebel, EK-
dc.contributor.authorRix, HW-
dc.date.accessioned2012-10-24T09:21:17Z-
dc.date.available2012-10-24T09:21:17Z-
dc.date.issued2004-
dc.identifier.citationASTRONOMICAL JOURNAL, 2004, 127 (5), pp. 2753-2770-
dc.identifier.issn0004-6256-
dc.identifier.urihttp://hdl.handle.net/2381/26084-
dc.language.isoEnglish-
dc.publisherUNIV CHICAGO PRESS-
dc.sourceWeb of Science-
dc.source.urihttp://webofknowledge.com-
dc.subjectScience & Technology-
dc.subjectPhysical Sciences-
dc.subjectAstronomy & Astrophysics-
dc.subjectgalaxy : halo-
dc.subjectglobular clusters : general-
dc.subjectglobular clusters : individual (Palomar 5)-
dc.subjectmethods : n-body simulations-
dc.subjectstellar dynamics-
dc.subjectFORCE-CALCULATION ALGORITHM-
dc.subjectDIGITAL SKY SURVEY-
dc.subjectSTAR-CLUSTERS-
dc.subjectDYNAMICAL EVOLUTION-
dc.subjectMILKY-WAY-
dc.subjectMASS FUNCTION-
dc.subjectTIDAL TAILS-
dc.subjectSATELLITES-
dc.subjectSYSTEMS-
dc.titleModeling the disruption of the globular cluster Palomar 5 by Galactic tides-
dc.typeJournal Article-
dc.identifier.doi10.1086/383214-
dc.description.irispid8790-
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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