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Please use this identifier to cite or link to this item: http://hdl.handle.net/2445/9179
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dc.contributor.authorSala Mirabet, Ferrancat
dc.contributor.authorTorra Roca, Jorgecat
dc.contributor.authorCortes, P.cat
dc.date.accessioned2009-08-21T07:58:42Z-
dc.date.available2009-08-21T07:58:42Z-
dc.date.issued1985cat
dc.identifier.issn0365-0138cat
dc.identifier.urihttp://hdl.handle.net/2445/9179-
dc.description.abstractHydrodynamical equations act as a link between the local observed magnitudes of galactic motion and the general ones accounting for the behaviour of the Galaxy as a whole. Constraints are set usually in order to use them even in the lower order hierarchy. The authors present in this paper the complete expressions up to their fourth order. These equations will be used in the next future in their general form taking into account both the expected increase of kinematic data that the astrometric mission Hipparcos will provide, and some recent results indicating the possibility to obtain estimates for the momenta gradients.eng
dc.format.extent18 p.cat
dc.format.mimetypeapplication/pdfeng
dc.language.isoengeng
dc.publisherEDP Sciencescat
dc.relation.isformatofReproducció digital del document publicat en format paper, proporcionada per NASA Astrophysics Data System http://adsabs.harvard.edu/cat
dc.relation.ispartofAstronomy and Astrophysics Supplement Series, 1985, vol. 62, p. 321-338.cat
dc.rights(c) The European Southern Observatory, 1985cat
dc.sourceArticles publicats en revistes (Física Quàntica i Astrofísica)-
dc.subject.classificationGalàxiescat
dc.subject.classificationDinàmicacat
dc.subject.classificationAstronomiacat
dc.subject.classificationEstadísticacat
dc.subject.otherGalactic dynamicseng
dc.subject.otherStatistical astronomyeng
dc.titleHigh order hydrodynamical equationseng
dc.typeinfo:eu-repo/semantics/articleeng
dc.typeinfo:eu-repo/semantics/publishedVersion-
dc.identifier.idgrec940cat
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess-
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