Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/26075
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dc.contributor.authorDehnen, W-
dc.contributor.authorBinney, J-
dc.date.accessioned2012-10-24T09:21:17Z-
dc.date.available2012-10-24T09:21:17Z-
dc.date.issued1998-3-1-
dc.identifier.citationMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1998, 294 (3), pp. 429-438-
dc.identifier.issn0035-8711-
dc.identifier.urihttp://hdl.handle.net/2381/26075-
dc.formatmetadata-
dc.language.isoEnglish-
dc.publisherBLACKWELL SCIENCE LTD-
dc.sourceWeb of Science-
dc.source.urihttp://webofknowledge.com-
dc.subjectScience & Technology-
dc.subjectPhysical Sciences-
dc.subjectAstronomy & Astrophysics-
dc.subjectGalaxy-
dc.subjectkinematics and dynamics-
dc.subjectGalaxy-
dc.subjectstructure-
dc.subjectGALACTIC DISK-
dc.subjectH-I-
dc.subjectROTATION CURVE-
dc.subjectGALAXY-
dc.subjectVELOCITY-
dc.subjectDENSITY-
dc.subjectHALO-
dc.subjectMOTION-
dc.titleMass models of the Milky Way-
dc.typeJournal Article-
dc.identifier.doi10.1046/j.1365-8711.1998.01282.x-
dc.description.irispid8774-
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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