The ALMA-PILS survey: detection of CH3NCO towards the low-mass protostar IRAS 16293−2422 and laboratory constraints on its formation

Author:

Ligterink N. F. W.12,Coutens A.3,Kofman V.1,Müller H. S. P.4,Garrod R. T.5,Calcutt H.6,Wampfler S. F.7,Jørgensen J. K.6,Linnartz H.1,van Dishoeck E. F.28

Affiliation:

1. Sackler Laboratory for Astrophysics, Leiden Observatory, Leiden University, PO Box 9513, NL-2300 RA Leiden, the Netherlands

2. Leiden Observatory, Leiden University, PO Box 9513, NL-2300 RA Leiden, the Netherlands

3. Department of Physics and Astronomy, University College London, Gower St., London WC1E 6BT, UK

4. I. Physikalisches Institut, Universität zu Köln, Zülpicher Str. 77, D-50937 Köln, Germany

5. Departments of Chemistry and Astronomy, University of Virginia, Charlottesville, VA 22904, USA

6. Centre for Star and Planet Formation, Niels Bohr Institute & Natural History Museum of Denmark, University of Copenhagen, Øster Voldgade 5-7, DK-1350 Copenhagen K., Denmark

7. Center for Space and Habitability, University of Bern, Sidlerstrasse 5, CH-3012 Bern, Switzerland

8. Max-Planck-Institut für Extraterrestrische Physik (MPE), Giessenbachstr. 1, D-85748 Garching, Germany

Funder

ERC

STFC

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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