Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/1208
DC FieldValueLanguage
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_US
dc.language.isoenen_US
dc.publisherCambridge : Cambridge University Pressen_US
dc.relation.ispartofProceedings of the International Astronomical Unionen_US
dc.subjectasteroid familiesen_US
dc.subjectasteroids: generalen_US
dc.subjectimpact processesen_US
dc.titleExcluding interlopers from asteroid familiesen_US
dc.typeConference Objecten_US
dc.relation.conferenceComplex Planetary Systems (S310 ; 2014 ; Namur)en_US
dc.relation.publicationIAU Symposium 310: Complex Planetary Systems, Namur (Belgium)en_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.issn1743-9213en_US
dc.description.rankM33en_US
dc.relation.firstpage174en_US
dc.relation.lastpage175en_US
dc.relation.volume9en_US
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.cerifentitytypePublications-
item.fulltextNo Fulltext-
item.grantfulltextnone-
item.openairetypeConference Object-
item.languageiso639-1en-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0001-6349-6881-
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