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The ground based leg for our ISO PNe: Spectroscopy

Published online by Cambridge University Press:  25 May 2016

F. Kerber ,
T. Köberl ,
H. Gratl  and
M. Roth
F. Kerber
Affiliation:
1Institut für Astronomie, Universität Innsbruck, Austria
T. Köberl
Affiliation:
1Institut für Astronomie, Universität Innsbruck, Austria
H. Gratl
Affiliation:
1Institut für Astronomie, Universität Innsbruck, Austria
M. Roth
Affiliation:
2Las Campanas Observatory, Carnegie Institution of Washington, Chile

Extract

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The Infrared Space Observatory (ISO) has to be regarded as the most powerful infrared facility that has ever been available to the astronomical community. In order to fully exploit the wealth of information contained in ISO data, one has to supplement the satellite observations with a ground-based campaign. In collaboration with the Kiel group, our group in Innsbruck is carrying out two observing programs with ISO. Our observations aim at the study of hot dust in bipolar PNe seen edge-on and in so-called “born-again” PNe.

Type
IV. Envelopes
Information
Symposium - International Astronomical Union , Volume 180: Planetary Nebulae , 1997 , pp. 246
Copyright
Copyright © Kluwer 1997