A&A 494, 623–636 (2009) Astronomy DOI: 10.1051/0004-6361:200810587 & c ESO 2009 Astrophysics Chemical modeling of L183 (L134N): an estimate of the ortho/para H2 ratio L. Pagani1, C. Vastel2, E. Hugo3, V. Kokoouline4,C.H.Greene5, A. Bacmann6, E. Bayet7, C. Ceccarelli6,R.Peng8, and S. Schlemmer3 1 LERMA & UMR8112 du CNRS, Observatoire de Paris, 61 Av. de l’Observatoire, 75014 Paris, France e-mail:
[email protected] 2 CESR, 9 avenue du colonel Roche, BP 44348, Toulouse Cedex 4, France e-mail:
[email protected] 3 I. Physikalisches Institut, Universität zu Köln, Zülpicher Strasse 77, 50937 Köln, Germany e-mail: [hugo;schlemmer]@ph1.uni-koeln.de 4 Department of Physics, University of Central Florida, Orlando, 32816, USA e-mail:
[email protected] 5 Department of Physics and JILA, University of Colorado, Boulder, Colorado 80309-0440, USA e-mail:
[email protected] 6 Laboratoire d’Astrophysique de Grenoble, Université Joseph Fourier, UMR 5571 du CNRS, 414 rue de la Piscine, 38041 Grenoble Cedex 09, France e-mail: [cecilia.ceccarelli;aurore.bacmann]@obs.ujf-grenoble.fr 7 Department of physics and astronomy, University College London, Gower street, London WC1E 6BT, UK e-mail:
[email protected] 8 Caltech Submillimeter Observatory, 111 Nowelo Street, Hilo, HI 96720, USA e-mail:
[email protected] Received 14 July 2008 / Accepted 6 October 2008 ABSTRACT + Context. The high degree of deuteration observed in some prestellar cores depends on the ortho-to-para H2 ratio through the H3 fractionation. Aims. We want to constrain the ortho/para H2 ratio across the L183 prestellar core.