An imaging line survey of OMC-1 to OMC-3

15 Mar 2020 Brinkmann N. Wyrowski F. Kauffmann J. Colombo D. Menten K. M. Tang X. D. Güsten R.

Aims: Our aim is to identify the dominant molecular cooling lines and characteristic emission features in the 1.3 mm window of distinct regions in the northern part of the Orion A molecular cloud. By defining and analysing template regions, we also intend to help with the interpretation of observations from more distant sources which cannot be easily spatially resolved... (read more)

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  • ASTROPHYSICS OF GALAXIES