Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/1208
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dc.contributor.authorRadović, Viktoren_US
dc.contributor.authorNovaković, Bojanen_US
dc.date.accessioned2022-09-23T17:57:50Z-
dc.date.available2022-09-23T17:57:50Z-
dc.date.issued2014-01-01-
dc.identifier.issn17439213en
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/1208-
dc.description.abstractTo study an asteroid family it is crucial to determine reliably the list of its members, i.e. to reduce the number of interlopers as much as possible. However, as the number of known asteroids increases fast it becomes more and more difficult to obtain robust list of members of an asteroid family. To cope with these challenges we are proposing a new approach that may help to significantly reduce presence of interlopers among the family members.en
dc.relation.ispartofProceedings of the International Astronomical Unionen
dc.subjectasteroid familiesen
dc.subjectasteroids: generalen
dc.subjectimpact processesen
dc.titleExcluding interlopers from asteroid familiesen_US
dc.typeConference Paperen_US
dc.identifier.doi10.1017/S1743921314008187-
dc.identifier.scopus2-s2.0-84956567740-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/84956567740-
dc.contributor.affiliationAstronomyen_US
dc.relation.firstpage174en
dc.relation.lastpage175en
dc.relation.volume9en
item.fulltextNo Fulltext-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.cerifentitytypePublications-
item.grantfulltextnone-
item.openairetypeConference Paper-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0001-6349-6881-
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