

Author: Immer K. Kauffmann J. Pillai T. Ginsburg A. Menten K. M.
Publisher: Edp Sciences
E-ISSN: 1432-0746|595|issue|A94-A94
ISSN: 0004-6361
Source: Astronomy & Astrophysics, Vol.595, Iss.issue, 2016-11, pp. : A94-A94
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Abstract
The central molecular zone at the center of our Galaxy is the best template to study star formation processes under extreme conditions, similar to those in high-redshift galaxies. We observed on-the-fly maps of para-H
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