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000007456 005__ 20250204104743.0
000007456 0247_ $$2DOI$$a10.25518/0037-9565.11808
000007456 037__ $$aSCART-2025-0087
000007456 100__ $$aFurst, T.
000007456 245__ $$aThe Star Formation History of the Young Open Cluster NGC 2244: Study of the Binary Fraction
000007456 260__ $$c2024
000007456 520__ $$aA star formation history (SFH) is the stellar record of the various processes that shaped a galaxy and star clusters since its birth to its current physical state. Studying the young open cluster NGC 2244, and in particular its massive stellar population, can improve our understanding of its formation mechanism, stellar evolution, feedback, and provide a basis for a better understanding of the formation of extragalactic star clusters. In this contribution, we present the first steps towards the derivation of the SFH of NGC 2244. We discuss the first results concerning the membership determination and the observed binary fractions of O- and B-type stars among NGC 2244. Finally, an overview of the forthcoming steps is also presented.
000007456 594__ $$aNO
000007456 700__ $$aMahy, L.
000007456 700__ $$aNazé, Y.
000007456 773__ $$c589-600$$n2$$pBulletin de la Société Royale des Sciences de Liège$$v93$$y2024
000007456 8560_ $$flaurent.mahy@ksb-orb.be
000007456 8564_ $$s3131505$$uhttp://publi2-as.oma.be/record/7456/files/Furst_bsrsl_2024.pdf
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000007456 905__ $$apublished in
000007456 980__ $$aREFERD