@prefix mdl: <http://data.loterre.fr/ark:/67375/MDL> .
@prefix skos: <http://www.w3.org/2004/02/skos/core#> .
@prefix dc: <http://purl.org/dc/terms/> .
@prefix xsd: <http://www.w3.org/2001/XMLSchema#> .

mdl:-CDX336Z0-T
  skos:prefLabel "rencontre proche"@fr, "close encounter"@en ;
  a skos:Concept ;
  skos:related mdl:-QB3DZJ30-1 .

mdl:-GMM48329-Z
  skos:prefLabel "amas jeune"@fr, "young cluster"@en ;
  a skos:Concept ;
  skos:broader mdl:-QB3DZJ30-1 .

mdl:-TTQ078XH-0
  skos:prefLabel "astronomie stellaire"@fr, "stellar astronomy"@en ;
  a skos:Concept ;
  skos:narrower mdl:-QB3DZJ30-1 .

mdl:-QB3DZJ30-1
  skos:hiddenLabel "Amas stellaires"@fr, "Star cluster"@en, "Amas stellaire"@fr, "amas stellaires"@fr, "star clusters"@en ;
  skos:inScheme mdl: ;
  skos:narrower mdl:-GMM48329-Z, mdl:-K2ZJZ6C9-Q, mdl:-LCCMF51V-9, mdl:-X2LHX4XP-G, mdl:-FLMK1HZC-N ;
  skos:exactMatch <https://en.wikipedia.org/wiki/Star_cluster>, <https://fr.wikipedia.org/wiki/Amas_stellaire> ;
  dc:modified "2022-10-10"^^xsd:date ;
  skos:definition "Un amas stellaire est une concentration locale d'étoiles d'origine commune et liées entre elles par la gravitation, dans un espace dont les dimensions peuvent atteindre 200 pc. Ces objets sont classés en plusieurs familles selon leur aspect ; ce sont, par compacité croissante : les associations stellaires, les amas ouverts et les amas globulaires. (Wikipedia, L'Encylopédie Libre, <a href=\"https://fr.wikipedia.org/wiki/Amas_stellaire\" target=\"_blank\">https://fr.wikipedia.org/wiki/Amas_stellaire</a>)"@fr, "Star clusters are large groups of stars. Two main types of star clusters can be distinguished: globular clusters are tight groups of ten thousand to millions of old stars which are gravitationally bound, while open clusters are more loosely clustered groups of stars, generally containing fewer than a few hundred members, and are often very young. Open clusters become disrupted over time by the gravitational influence of giant molecular clouds as they move through the galaxy, but cluster members will continue to move in broadly the same direction through space even though they are no longer gravitationally bound; they are then known as a stellar association, sometimes also referred to as a moving group. (Wikipedia, The Free Encyclopedia, <a href=\"https://en.wikipedia.org/wiki/Star_cluster\" target=\"_blank\">https://en.wikipedia.org/wiki/Star_cluster</a>)"@en ;
  skos:prefLabel "star cluster"@en, "amas stellaire"@fr ;
  skos:related mdl:-CDX336Z0-T, mdl:-CFWB4C0D-B ;
  a skos:Concept ;
  skos:broader mdl:-TTQ078XH-0 .

mdl:-LCCMF51V-9
  skos:prefLabel "amas globulaire"@fr, "globular cluster"@en ;
  a skos:Concept ;
  skos:broader mdl:-QB3DZJ30-1 .

mdl:-X2LHX4XP-G
  skos:prefLabel "amas stellaire extragalactique"@fr, "extragalactic star cluster"@en ;
  a skos:Concept ;
  skos:broader mdl:-QB3DZJ30-1 .

mdl:-CFWB4C0D-B
  skos:prefLabel "color-magnitude diagram"@en, "diagramme magnitude-couleur"@fr ;
  a skos:Concept ;
  skos:related mdl:-QB3DZJ30-1 .

mdl: a skos:ConceptScheme .
mdl:-K2ZJZ6C9-Q
  skos:prefLabel "association stellaire"@fr, "stellar association"@en ;
  a skos:Concept ;
  skos:broader mdl:-QB3DZJ30-1 .

mdl:-FLMK1HZC-N
  skos:prefLabel "amas ouvert"@fr, "open cluster"@en ;
  a skos:Concept ;
  skos:broader mdl:-QB3DZJ30-1 .