Modelling the abundance structure of isocyanic acid (HNCO) towards the low-mass solar type protostar IRAS 16293

Modelling the abundance structure of isocyanic acid (HNCO) towards the low-mass solar type protostar IRAS 16293–2422

Published:2018-11-03 Issue:2 Volume:483 Page:2014-2030
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
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Author:

Hernández-Gómez Antonio¹²^ORCID,Sahnoun Emna³⁴^ORCID,Caux Emmanuel²^ORCID,Wiesenfeld Laurent⁴⁵^ORCID,Loinard Laurent¹⁶^ORCID,Bottinelli Sandrine²^ORCID,Hammami Kamel³^ORCID,Menten Karl M⁷^ORCID

Affiliation:

1. Instituto de Radioastronomía y Astrofísica, Universidad Nacional Autónoma de México, Morelia 58089, Mexico

2. IRAP, Université de Toulouse, CNRS, UPS, CNES, Toulouse, France

3. Laboratory of Atomic Molecular Spectroscopy and Applications, Department of Physics, Faculty of Science, University Tunis El Manar, Campus Universities, 1060 Tunis, Tunisia

4. IPAG, Université Grenoble Alpes, CNRS, F-38000 Grenoble, France

5. Laboratoire Aimé-Cotton, Université Paris-Saclay, CNRS, Orsay, France

6. Instituto de Astronomía, Universidad Nacional Autónoma de México, Apartado Postal 70-264, CdMx C.P. 04510, Mexico

7. Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany

Funder

Canadian Space Agency

Alberta Livestock and Meat Agency

European School of Oncology

National Science Foundation

National Institutes of Natural Sciences

National Research Council Canada

Korea Astronomy and Space Science Institute