Extragalactic Planetary Nebula: Methods of Discovery Using Infrared Photometry

García-Lario, Pedro; Bayo, Amelia; Alfageme, Carlos

doi:10.1007/11604792_8

Pedro García-Lario⁴,
Amelia Bayo⁴ &
Carlos Alfageme⁴

Part of the book series: ESO ASTROPHYSICS SYMPOSIA European Southern Observatory ((ESO))

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Abstract

Methods for discovering new planetary nebulae based on their characteristic near-, mid- and far-infrared photometric colours are presented. We describe the methods and review the results obtained for Galactic sources. Their possible application to extragalactic searches is discussed.

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Authors and Affiliations

ESAC/ISO Data Centre, Apartado de Correos 50727, Madrid, E-28080, Spain
Pedro García-Lario, Amelia Bayo & Carlos Alfageme

Authors

Pedro García-Lario
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Amelia Bayo
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Carlos Alfageme
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Editors and Affiliations

NOAO, 950 N Cherry Ave, Tucson, AZ, 85719, USA
L. Stanghellini
European Southern Observatory, Karl-Schwarzschild-Str. 2, Garching, 85748, Germany
J. R. Walsh
Kapteyn Astronomical Institute, University of Groningen, 800, Groningen, AV, 9700, The Netherlands
N. G. Douglas

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García-Lario, P., Bayo, A., Alfageme, C. (2006). Extragalactic Planetary Nebula: Methods of Discovery Using Infrared Photometry. In: Stanghellini, L., Walsh, J.R., Douglas, N.G. (eds) Planetary Nebulae Beyond the Milky Way. ESO ASTROPHYSICS SYMPOSIA European Southern Observatory. Springer, Berlin, Heidelberg . https://doi.org/10.1007/11604792_8

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DOI: https://doi.org/10.1007/11604792_8
Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-540-31011-2
Online ISBN: 978-3-540-34270-0
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