The Red Giant Branch Bump

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dc.creatorRiello, M.
dc.creatorPiotto, G.
dc.creatorRecio-Blanco, A.
dc.creatorCassisi, S.
dc.creatorSalaris, M.
dc.date2003-03-13
dc.date.accessioned2026-07-07T02:07:55Z
dc.date.available2026-07-07T02:07:55Z
dc.descriptionWe present a comparison between theoretical models and the observed magnitude difference between the horizontal branch and the red giant branch bump for a sample of 53 clusters. We find a general agreement, though some discrepancy is still present at the two extremes of the metallicity range of globular clusters.
dc.description2 pages, 1 figure, A.S.P. Conf. Ser., in press in Vol. 296, 2003
dc.identifierhttps://arxiv.org/abs/astro-ph/0303295
dc.identifierhttp://arxiv.org/abs/astro-ph/0303295
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5857
dc.subjectAstrophysics
dc.titleThe Red Giant Branch Bump
dc.typetext

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