UV photodesorption of interstellar CO ice analogues: from subsurface excitation to surface desorption
Abstract
Carbon monoxide is after H2 the most abundant molecule identified in the interstellar medium (
* Corresponding authors
a
UPMC Univ. Paris 6, Laboratoire de Physique Moléculaire pour l'Atmosphère et l'Astrophysique (LPMAA) – CNRS UMR 7092, F-75252 Paris, France
E-mail:
mathieu.bertin@upmc.fr
b Sackler Laboratory for Astrophysics, Leiden Observatory, Leiden University, P.O. Box 9513, NL-2300 RA Leiden, The Netherlands
c Université Paris Sud 11, Laboratoire de Chimie Physique (LCP) – CNRS UMR 8000, F-91400 Orsay, France
d Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, USA
Carbon monoxide is after H2 the most abundant molecule identified in the interstellar medium (
M. Bertin, E. C. Fayolle, C. Romanzin, K. I. Öberg, X. Michaut, A. Moudens, L. Philippe, P. Jeseck, H. Linnartz and J. Fillion, Phys. Chem. Chem. Phys., 2012, 14, 9929 DOI: 10.1039/C2CP41177F
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