Magellanic Clouds Planetary Nebulae: an updated view on stellar evolution and populations

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dc.creatorStanghellini, Letizia
dc.creatorShaw, Richard A.
dc.creatorMutchler, Max
dc.date2001-03-05
dc.date.accessioned2026-07-07T01:57:53Z
dc.date.available2026-07-07T01:57:53Z
dc.descriptionPlanetary Nebulae (PNs) in the Magellanic Clouds are studied to understand stellar populations and evolution of low- and intermediate-mass stars in different chemical environments. Using HST observations from our LMC and SMC PN morphological survey and from the HST Data Archive, we look at the relations between PN morphology and their evolution and populations. In this paper we show some of our recent results on these relations, in an historical context.
dc.descriptionInvited talk. Proceedings of the conference "Ionized Gaseous Nebulae", Mexico City, November 21- 24, 2000; RMAA, in press
dc.identifierhttps://arxiv.org/abs/astro-ph/0103076
dc.identifierhttp://arxiv.org/abs/astro-ph/0103076
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2559
dc.subjectAstrophysics
dc.titleMagellanic Clouds Planetary Nebulae: an updated view on stellar evolution and populations
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