The ALMA-PILS Survey: Isotopic Composition of Oxygen-Containing Complex Organic Molecules Toward IRAS 16293–2422B J
Astronomy & Astrophysics manuscript no. ms c ESO 2018 August 28, 2018 The ALMA-PILS survey: Isotopic composition of oxygen-containing complex organic molecules toward IRAS 16293–2422B J. K. Jørgensen1, H. S. P. Müller2, H. Calcutt1, A. Coutens3, M. N. Drozdovskaya4, K. I. Öberg5 M. V. Persson6, V. Taquet7, E. F. van Dishoeck8; 9, and S. F. Wampfler4 1 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 2 I. Physikalisches Institut, Universität zu Köln, Zülpicher Str. 77, 50937 Köln, Germany 3 Laboratoire d’astrophysique de Bordeaux, Univ. Bordeaux, CNRS, B18N, allée Geoffroy Saint-Hilaire, 33615 Pessac, France 4 Center for Space and Habitability (CSH), University of Bern, Sidlerstrasse 5, CH-3012 Bern, Switzerland 5 Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA 6 Department of Earth and Space Sciences, Chalmers University of Technology, Onsala Space Observatory, 439 92 Onsala, Sweden 7 INAF-Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I-50125 Firenze, Italy 8 Leiden Observatory, Leiden University, PO Box 9513, NL-2300 RA Leiden, The Netherlands 9 Max-Planck Institut für Extraterrestrische Physik (MPE), Giessenbachstr. 1, 85748 Garching, Germany August 28, 2018 ABSTRACT Context. One of the important questions of astrochemistry is how complex organic molecules, including potential prebiotic species, are formed in the envelopes around embedded protostars. The abundances of minor isotopologues of a molecule, in particular the D- and 13C-bearing variants, are sensitive to the densities, temperatures and time-scales characteristic of the environment in which they form, and can therefore provide important constraints on the formation routes and conditions of individual species.
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