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UV-NIR spectra of two planetary nebulae with X-Shooter

Published online by Cambridge University Press:  30 August 2012

Cezary Szyszka ,
Jeremy R. Walsh  and
Albert A. Zijlstra
Cezary Szyszka
Affiliation:
Jodrell Bank Centre for Astrophysics, University of Manchester, United Kingdom
Jeremy R. Walsh
Affiliation:
European Southern Observatory, Garching, Germany
Albert A. Zijlstra
Affiliation:
Jodrell Bank Centre for Astrophysics, University of Manchester, United Kingdom
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Abstract

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The ESO VLT spectrograph X-shooter is currently the only one capable of observing the range from 330 nm up to 2.5 μm in a single shot. X-shooter is very suitable for study of the many diagnostic emission lines in PN providing a uniform flux scale at medium resolution over a large instantaneous wavelength range. Spectroscopy of two contrasting PNe, NGC 6302 and M 2-9, were observed and methods explored for identification of the many fitted emission lines.

Keywords

planetary nebulae: individual (M2-9, NGC 6302)techniques: spectroscopic
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Symposium S283: Planetary Nebulae: An Eye to the Future , July 2011 , pp. 508 - 509
Copyright
Copyright © International Astronomical Union 2012

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