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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/939
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dc.contributor.authorKovačević, Anđelkaen_US
dc.date.accessioned2022-08-16T11:22:34Z-
dc.date.available2022-08-16T11:22:34Z-
dc.date.issued2005-01-01-
dc.identifier.issn00046361en
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/939-
dc.description.abstractHere I present a new attempt to determine the mass of (4) Vesta, based on its close approaches with relatively well observed minor planets: (3057) Malaren, (5205) 1988CU7, (8331) Dawkins and (21225) 1995GQ1. The obtained values for the mass of (4) Vesta are comparable with earlier determined ones.en
dc.relation.ispartofAstronomy and Astrophysicsen
dc.subjectAstrometryen
dc.subjectCelestial mechanicsen
dc.titleDetermination of the mass of (4) Vesta based on new close approachesen_US
dc.typeArticleen_US
dc.identifier.doi10.1051/0004-6361:20035872-
dc.identifier.scopus2-s2.0-12844276630-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/12844276630-
dc.contributor.affiliationAstronomyen_US
dc.relation.firstpage319en
dc.relation.lastpage325en
dc.relation.volume430en
dc.relation.issue1en
item.fulltextNo Fulltext-
item.openairetypeArticle-
item.grantfulltextnone-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.cerifentitytypePublications-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0001-5139-1978-
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