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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/2777
DC FieldValueLanguage
dc.contributor.authorNovaković, Bojanen_US
dc.contributor.authorH.h., Hsiehen_US
dc.contributor.authorA., Cellinoen_US
dc.date.accessioned2025-10-17T08:48:53Z-
dc.date.available2025-10-17T08:48:53Z-
dc.date.issued2012-
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/2777-
dc.description.abstractHere we present our results obtained by applying diferent methods in order to establish a firm link between the main-belt comets (MBCs) and colisionally-formed asteroid families (AFs), i.e, to possibly find additional line of evidence supporting the hypothesis that MBCs may be preferentially found among the members of young AFs.en_US
dc.language.isoenen_US
dc.publisherMadriden_US
dc.titleLinking main-belt comets to asteroid familiesen_US
dc.typeConference Objecten_US
dc.relation.conferenceEuropean Planetary Science Congress EPSC (7 ; 2012 ; Madrid)en_US
dc.relation.publicationEuropean Planetary Science Congress (EPSC2012)en_US
dc.identifier.urlhttp://meetingorganizer.copernicus.org/EPSC2012/EPSC2012-746.pdf-
dc.description.rankM34en_US
dc.relation.firstpage[Abstract no.] 746en_US
item.openairetypeConference Object-
item.fulltextNo Fulltext-
item.languageiso639-1en-
item.cerifentitytypePublications-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.grantfulltextnone-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0001-6349-6881-
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