The lower mass function of young open clusters

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dc.creatorBouvier, J.
dc.creatorMoraux, E.
dc.creatorStauffer, J. R.
dc.creatorNavascues, D. Barrado y
dc.creatorCuillandre, J. -C.
dc.date2002-09-10
dc.date.accessioned2026-07-07T02:05:04Z
dc.date.available2026-07-07T02:05:04Z
dc.descriptionWe report new estimates for the lower mass function of 5 young open clusters spanning an age range from 80 to 150 Myr. In all studied clusters, the mass function across the stellar/substellar boundary (~0.072 Mo) and up to 0.4 Mo is consistent with a power-law with an exponent alpha of -0.5 +/- 0.1, i.e., dN/dM ~ M**(-0.5).
dc.description8 pages, 4 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0209178
dc.identifierhttp://arxiv.org/abs/astro-ph/0209178
dc.identifierIAU Symp.211 "Brown Dwarfs", E.L. Martin ed., 2002
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4993
dc.subjectAstrophysics
dc.titleThe lower mass function of young open clusters
dc.typetext

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