The Galactic Bulge: The Stellar and Planetary Nebulae Populations

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dc.creatorCuisinier, F.
dc.creatorKoppen, J.
dc.creatorAcker, A.
dc.creatorMaciel, W. J.
dc.date2001-01-12
dc.date.accessioned2026-07-07T01:57:22Z
dc.date.available2026-07-07T01:57:22Z
dc.descriptionWe compare abundances patterns in the Bulge for elements observed in stars and in planetary nebulae. Some alpha elements, like Mg and Ti, are overabundant respect to Fe, and others are not, like He, O, Si, S, Ar, Ca. The first ones favor a quick evolution of the Galactic Bulge, and the seconds a much slower one.
dc.descriptionTo be published in Rev.Mex. A&A, Conf. Series. Proceedings of the conference ``Ionized Gaseous Nebulae'', held in Mexico City, Nov. 21-24, 2000
dc.identifierhttps://arxiv.org/abs/astro-ph/0101215
dc.identifierhttp://arxiv.org/abs/astro-ph/0101215
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2359
dc.subjectAstrophysics
dc.titleThe Galactic Bulge: The Stellar and Planetary Nebulae Populations
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