Please use this identifier to cite or link to this item:
https://research.matf.bg.ac.rs/handle/123456789/939| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Kovačević, Anđelka | en_US |
| dc.date.accessioned | 2022-08-16T11:22:34Z | - |
| dc.date.available | 2022-08-16T11:22:34Z | - |
| dc.date.issued | 2005-01-01 | - |
| dc.identifier.issn | 00046361 | en |
| dc.identifier.uri | https://research.matf.bg.ac.rs/handle/123456789/939 | - |
| dc.description.abstract | Here 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.ispartof | Astronomy and Astrophysics | en |
| dc.subject | Astrometry | en |
| dc.subject | Celestial mechanics | en |
| dc.title | Determination of the mass of (4) Vesta based on new close approaches | en_US |
| dc.type | Article | en_US |
| dc.identifier.doi | 10.1051/0004-6361:20035872 | - |
| dc.identifier.scopus | 2-s2.0-12844276630 | - |
| dc.identifier.url | https://api.elsevier.com/content/abstract/scopus_id/12844276630 | - |
| dc.contributor.affiliation | Astronomy | en_US |
| dc.relation.firstpage | 319 | en |
| dc.relation.lastpage | 325 | en |
| dc.relation.volume | 430 | en |
| dc.relation.issue | 1 | en |
| item.cerifentitytype | Publications | - |
| item.openairetype | Article | - |
| item.fulltext | No Fulltext | - |
| item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
| item.grantfulltext | none | - |
| crisitem.author.dept | Astronomy | - |
| crisitem.author.orcid | 0000-0001-5139-1978 | - |
| Appears in Collections: | Research outputs | |
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