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The past, present and future of Galactic planetary nebula surveys

Published online by Cambridge University Press:  30 August 2012

Quentin A. Parker ,
David J. Frew ,
Agnes Acker  and
Brent Miszalski
Quentin A. Parker
Affiliation:
Department of Physics and Astronomy, Macquarie University, Sydney, NSW 2109, Australia Macquarie University Research Centre in Astronomy, Astrophysics & Astrophotonics Australian Astronomical Observatory, PO Box 296, Epping, NSW 1710, Australia email: [email protected]
David J. Frew
Affiliation:
Department of Physics and Astronomy, Macquarie University, Sydney, NSW 2109, Australia Macquarie University Research Centre in Astronomy, Astrophysics & Astrophotonics
Agnes Acker
Affiliation:
Observatoire Astronomique de Strasbourg, 11 rue de l' Université, 67000 Strasbourg, France
Brent Miszalski
Affiliation:
South African Astronomical Observatory, P.O. Box 9, Observatory, 7935, South Africa
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Abstract

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Over the last decade Galactic planetary nebula discoveries have entered a golden age due to the emergence of high sensitivity, high resolution narrow-band surveys of the Galactic plane. These have been coupled with access to complimentary, deep, multi-wavelength surveys across near-IR, mid-IR and radio regimes in particular from both ground-based and space-based telescopes. These have provided powerful diagnostic and discovery capabilities. In this review these advances are put in the context of what has gone before, what we are uncovering now and through the window of opportunity that awaits in the future. The astrophysical potential of this brief but key phase of late stage stellar evolution is finally being realised.

Keywords

Planetary nebulae: generalcatalogssurveysinfrared: starsradio continuum: starsISM: generalGalaxy: evolution
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Symposium S283: Planetary Nebulae: An Eye to the Future , July 2011 , pp. 9 - 16
Copyright
Copyright © International Astronomical Union 2012

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