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Line Observations of NGC1068, NGC1808 and Other Southern Galaxies with FAST, the MPE NIR Fabry-Perot Imaging Spectrometer

Published online by Cambridge University Press:  03 August 2017

A. Krabbe ,
V. Rotaciuc ,
S. Drapatz  and
R Genzel
A. Krabbe
Affiliation:
Max-Planck-Institut für Physik und Astrophysik Institut für extraterrestrische Physik D-8046 Garching bei München, Federal Republic of Germany
V. Rotaciuc
Affiliation:
Max-Planck-Institut für Physik und Astrophysik Institut für extraterrestrische Physik D-8046 Garching bei München, Federal Republic of Germany
S. Drapatz
Affiliation:
Max-Planck-Institut für Physik und Astrophysik Institut für extraterrestrische Physik D-8046 Garching bei München, Federal Republic of Germany
R Genzel
Affiliation:
Max-Planck-Institut für Physik und Astrophysik Institut für extraterrestrische Physik D-8046 Garching bei München, Federal Republic of Germany

Abstract

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Images with subarcsec spatial resolution in the light of near infrared atomic (Brγ) and molecular (1-0 and 2-1 S(1)) hydrogen emission lines have been obtained for some southern starburst and Seyfert galaxies for the first time. The data were obtained with the Max-Planck-Institut für extraterrestrische Physik (MPE) near-infrared array spectrometer (image scale 0.8″ /px, resolving power 950) during an observation run in January 1990 at the ESO/MPI 2.2m telescope. We investigated NGC253, NGC5253, Cen A, M83, LMC, He2-10, NGC1068 and NGC1808. Some results on the last two galaxies are presented.

Type
IX- Galaxy Nuclei
Information
Symposium - International Astronomical Union , Volume 146: Dynamics of Galaxies and their Molecular Cloud Distributions , 1991 , pp. 310
Copyright
Copyright © Kluwer 1991