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Planetary Nebulae: Sources of Enlightenment
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In this review/tutorial we explore planetary nebulae as a stage in the evolution of low-to-intermediate-mass stars, as major contributors to the mass and chemical enrichment of the interstellar medium, and as astrophysical laboratories. We discuss many observed properties of planetary nebulae, placing particular emphasis on element abundance determinations and comparisons with theoretical predictions. Dust and molecules associated with planetary nebulae are considered as well. We then examine distances, binarity, and planetary nebula morphology and evolution. We end with mention of some of the advances that will be enabled by future observing capabilities.
Forward citations
Cited by 3 Pith papers
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Unveiling compact planetary nebulae: Broad-band survey analysis and LAMOST confirmation
A new Gaia plus Pan-STARRS color-color selection method identifies compact planetary nebulae and yields the discovery of the high-ionization PN J020808.63+491401.0, confirmed by LAMOST spectroscopy and Cloudy modeling.
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Dynamical formation of long-period exoplanets systems in evolving binary stars
MESA+REBOUND simulations show that stellar mass loss in a wide binary destabilizes S-type multi-planet systems and pushes surviving giants to long-period orbits.
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