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Line observations of the 30-Dor complex and N159A5 with the MPE imaging NIR spectrometer FAST

Published online by Cambridge University Press:  19 July 2016

A. Krabbe ,
J. Storey ,
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, FR Germany
J. Storey
Affiliation:
Max-Planck-Institut für Physik und Astrophysik, Institut für extraterrestrische Physik, D-8046 Garching bei München, FR Germany
V. Rotaciuc
Affiliation:
Max-Planck-Institut für Physik und Astrophysik, Institut für extraterrestrische Physik, D-8046 Garching bei München, FR Germany
S. Drapatz
Affiliation:
Max-Planck-Institut für Physik und Astrophysik, Institut für extraterrestrische Physik, D-8046 Garching bei München, FR Germany
R. Genzel
Affiliation:
Max-Planck-Institut für Physik und Astrophysik, Institut für extraterrestrische Physik, D-8046 Garching bei München, FR Germany

Abstract

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Images with subarcsec spatial resolution in the light of near-infrared atomic (Bry) and molecular hydrogen H2 (S(1) v=1-0) emission lines were obtained for some extended, pointlike objects in the Large Magellanic Cloud (LMC) for the first time. We used the Max-Planck-Institut für extraterrestrische Physik (MPE) near-infrared array spectrometer FAST (image scale 0.8”/pix, spectral resolving power 950) at the ESO/MPI 2.2m telescope, La Silla. We present some results on the 30-Dor complex and N159A5.

Type
Star Formation and Clustering
Information
Symposium - International Astronomical Union , Volume 148: The Magellanic Clouds , 1991 , pp. 205 - 206
Copyright
Copyright © Kluwer 1991 

References

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