Accuracy of Star Cluster Parameters from Integrated UBVRI Photometry

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dc.creatorNarbutis, D.
dc.creatorBridzius, A.
dc.creatorStonkute, R.
dc.creatorVansevicius, V.
dc.date2007-12-23
dc.date.accessioned2026-07-07T11:13:55Z
dc.date.available2026-07-07T11:13:55Z
dc.descriptionWe study the capability of the UBVRI photometric system to quantify star clusters in terms of age, metallicity, and color excess by their integrated photometry. The well known age-metallicity-extinction degeneracy was analyzed for various parameter combinations, assuming different levels of photometric accuracy. We conclude that the UBVRI photometric system enables us to estimate star cluster parameters over a wide range, if the overall photometric accuracy is better than ~0.03 mag.
dc.description9 pages, 8 figures
dc.identifierhttps://arxiv.org/abs/0712.3959
dc.identifierhttp://arxiv.org/abs/0712.3959
dc.identifierBalticAstron.16:421-429,2007
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/191887
dc.subjectAstrophysics
dc.titleAccuracy of Star Cluster Parameters from Integrated UBVRI Photometry
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