Open Clusters in the log Age vs. M_V plane

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dc.creatorBellazzini, M.
dc.creatorPerina, S.
dc.creatorGalleti, S.
dc.creatorFederici, L.
dc.creatorBuzzoni, A.
dc.creatorPecci, F. Fusi
dc.date2007-11-05
dc.date2007-11-08
dc.date.accessioned2026-07-07T08:41:15Z
dc.date.available2026-07-07T08:41:15Z
dc.descriptionIn the log Age vs. integrated absolute magnitude (M_V) plane, the open clusters of the Milky Way form a well-defined band parallel to theoretical sequences decribing the passive evolution of Simple Stellar Populations and display a pretty sharp upper threshold in mass (M ~ 2X 10^4 M_{sun}) over a 4 dex range of ages.
dc.description3 pages, 3 greyscale figures. Proceedings of the workshop "XXI Century challenges for stellar evolution", held in Cefalu' (Sicily, Italy), August 29 - September 2, 2007; S. Cassisi and M. Salaris Eds. To be published in Mem. SAIt Vol. 79 No. 2. A few relevant changes to include fundamental references that were neglected in the original manuscript
dc.identifierhttps://arxiv.org/abs/0711.0702
dc.identifierhttp://arxiv.org/abs/0711.0702
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/141624
dc.subjectAstrophysics
dc.titleOpen Clusters in the log Age vs. M_V plane
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