Investigating the process of star formation in young LMC star clusters

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dc.creatorJohnson, R. A.
dc.creatorBeaulieu, S. F.
dc.creatorElson, R. A. W.
dc.creatorGilmore, G.
dc.creatorTanvir, N.
dc.creatorSantiago, B.
dc.date1999-07-19
dc.date1999-07-29
dc.date.accessioned2026-07-07T02:32:34Z
dc.date.available2026-07-07T02:32:34Z
dc.descriptionThe rich star clusters in the Large Magellanic Cloud (LMC) are ideal for studying the process of star formation. Here we focus on the determination of age spreads amongst the massive stars in two young clusters, NGC1818 and NGC1805. We present colour magnitude diagrams (derived from HST data) for these clusters, and discuss the difficulties in age spread determination.
dc.descriptionreplaced with revised figures 4 pages, to appear in Stellar Clusters and Associations: Convection, rotation and dynamos, May 1999, Sicily, ed. R. Pallavicini
dc.identifierhttps://arxiv.org/abs/astro-ph/9907246
dc.identifierhttp://arxiv.org/abs/astro-ph/9907246
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/14509
dc.subjectAstrophysics
dc.titleInvestigating the process of star formation in young LMC star clusters
dc.typetext

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