A new grid of evolutionary synthesis models

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dc.creatorMollá, M.
dc.creatorGarcía-Vargas, M. L.
dc.creatorBressan, Alessandro
dc.creatorGómez-Alvarez, Pedro
dc.date2007-11-20
dc.date.accessioned2026-07-07T08:44:00Z
dc.date.available2026-07-07T08:44:00Z
dc.descriptionWe present new evolutionary synthesis models for Single Stellar Populations covering a wide range in age and metallicity. The most important difference with existing models is the use of NLTE atmosphere models for the hot stars (O, B, WR, post-AGB stars, and planetary nebulae) that have an important impact in the stellar cluster's ionizing spectra.
dc.description2 pages, 1 figure, proceedings of the conference Pathways Through an Eclectic Universe, Eds. T.Mahoney, A. Vazdekis & J. Knapen, Tenerife 2007
dc.identifierhttps://arxiv.org/abs/0711.3141
dc.identifierhttp://arxiv.org/abs/0711.3141
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/142511
dc.subjectAstrophysics
dc.titleA new grid of evolutionary synthesis models
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