Resolved and unresolved populations: statistics and synthesis models

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dc.creatorCervino, M.
dc.date2002-06-11
dc.date.accessioned2026-07-07T02:03:55Z
dc.date.available2026-07-07T02:03:55Z
dc.descriptionIn this contribution, I present the 90% confidence limits on the diagnostic diagrams of EW(WR bump) and L(WR bump)/L(Hb) ratio vs. EW(Hb) resulting from evolutionary synthesis models that include the statistical dispersion due to finite stellar populations in real star forming regions.
dc.description2 pages, 2 figures, To be presented in IAU Symp. 212
dc.identifierhttps://arxiv.org/abs/astro-ph/0206169
dc.identifierhttp://arxiv.org/abs/astro-ph/0206169
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4561
dc.subjectAstrophysics
dc.titleResolved and unresolved populations: statistics and synthesis models
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