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Clues on post-Asymptotic Giant Branch Evolution and Planetary Nebulae Populations from the Magellanic Clouds

Letizia Stanghellini
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Abstract

The recent HST optical images, and the optical and ultraviolet spectra, of Magellanic planetary nebulae (PNe), together with the large data-base that has been collected in the past decade, allows unprecedented insight in the evolution of PNe and their central stars. In this paper we present a selection of recent results: The analysis of PN morphology, both in the optical and ultra-violet emission lines; the relation between nebular morphology and the chemistry produced by stellar evolution; the direct determination of the transition time from observations; and the study of the nature and evolutionary stage of the components of the planetary nebula luminosity function.

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Letizia Stanghellini. 2004-09-07. Clues on post-Asymptotic Giant Branch Evolution and Planetary Nebulae Populations from the Magellanic Clouds. https://arxiv.org/abs/astro-ph/0409165

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