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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/2621
DC FieldValueLanguage
dc.contributor.authorKnežević, Zoranen_US
dc.contributor.authorMilani, Andreaen_US
dc.contributor.authorNovaković, Bojanen_US
dc.contributor.authorCelino, A.en_US
dc.contributor.authorSpoto, F.en_US
dc.contributor.authorPaolicchi, P.en_US
dc.date.accessioned2025-09-20T16:53:16Z-
dc.date.available2025-09-20T16:53:16Z-
dc.date.issued2014-
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/2621-
dc.language.isoenen_US
dc.publisherInternational Astronomical Union IAUen_US
dc.titleBig cratering families: how to match dynamics with physicsen_US
dc.typeConference Objecten_US
dc.relation.conferenceIAU Symposium: Complex Planetary Systems (310 ; 2014 ; Namur)en_US
dc.relation.publicationIAU Symposium 310: Complex Planetary Systems, Namur (Belgium), Abstractsen_US
dc.contributor.affiliationAstronomyen_US
dc.description.rankM34en_US
dc.relation.firstpage35en_US
dc.relation.lastpage35en_US
item.languageiso639-1en-
item.cerifentitytypePublications-
item.grantfulltextnone-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextNo Fulltext-
item.openairetypeConference Object-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0001-6349-6881-
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