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2.3. Mosaic-mapping of very extended objects in (sub)millimetre and near-infrared

Published online by Cambridge University Press:  25 May 2016

Sabine Philipp  and
Robert Zylka
Sabine Philipp
Affiliation:
Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany Institut für Theoretische Astrophysik, Tiergartenstrasse 15, 69121 Heidelberg, Germany
Robert Zylka
Affiliation:
Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany Institut für Theoretische Astrophysik, Tiergartenstrasse 15, 69121 Heidelberg, Germany

Extract

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The details of current and past star formation episodes and the stellar content of the central parsecs of our galaxy are still not very well known (Mezger et al., 1996). We have therefore begun an observing program to study star formation processes in the nuclear bulge. Here we discuss the technical aspects of this program, while the scientific goals are presented by Zylka et al. (1997).

Type
Part I. Stellar Cluster, Star Formation
Information
Symposium - International Astronomical Union , Volume 184: The Central Regions of the Galaxy and Galaxies , 1998 , pp. 63 - 64
Copyright
Copyright © Kluwer 1998 

References

Mezger, P.G., Duschl, W.J., Zylka, R., 1996, A&AR, 7, 4.Google Scholar
Zylka, R. et al., 1997, in these proceedings.Google Scholar