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Planetary nebulae populations in external galaxies

Published online by Cambridge University Press:  30 August 2012

Magda Arnaboldi
Magda Arnaboldi*
Affiliation:
European Southern Observatory, Karl-Schwarzchild-Strasse 2, 85748 Garching bei München, Germany email: marnabol@eso.org INAF, Osservatorio Astronomico di Pino Torinese, I-10025 Pino Torinese, Italy
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Abstract

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This review highlights the properties of the planetary nebulae in external galaxies as tracers of light, of the stellar population properties, and of the distances and kinematics of the parent galaxies. Recent results on the kinematics of the outer regions in giant elliptical galaxies and on the luminosity specific PN numbers (the α parameter) in these systems are presented, based on current surveys of planetary nebulae with the Planetary Nebulae Spectrograph (PN.S) and other instruments. Finally a brief discussion is given of planetary nebulae as tracers of the diffuse light in the nearby clusters, such as Virgo and Hydra I.

Keywords

planetary nebulae: generalgalaxies: kinematics and dynamics
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Symposium S283: Planetary Nebulae: An Eye to the Future , July 2011 , pp. 267 - 274
Copyright
Copyright © International Astronomical Union 2012

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