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Lis (CSO), David Teyssier (LERMA), Edith Falgarone (LERMA), Emmanuel Dartois (IAS), Eric Herbst (OHIO STATE UNIVERSITY), Francois Boulanger (IAS), Harshal Gupta (JPL), Jacek Krelowski, Javier R.Goicoechea (CAB-INTA, Jesus Martin-Pintado (IEM), John Black (oso), John C. Pearson (JPL), Jonas Zmuidzinas (CSO), Jos\\'e Cernicharo (CAB-INTA, J\\\"urgen Stutzki, Karl Menten (MPIfR), K. Klein, L. A Samoska (JPL), Maja Kazmierczak, Maryvonne Gerin (LERMA), M. De Luca (LERMA), Michel P\\'erault (LERMA), Mirisloaw Schmidt, Morvan Salez (LERMA), Patrick Hennebelle (LERMA), Paul B. Rimmer (OHIO STATE UNIVERSITY), Paule Sonnentrucker, Paul F. Goldsmith (JPL), Pierre Encrenaz (LERMA), Pierre Hily-Blant (LAOG), Raquel Monje (CSO), Ren\\'e Plume, Robert Kolos, Russ Shipman (SRON), Sabine Philipp-May (MpIfR), Shan Shan Yu (JPL), Stephan Schlemmer, Thomas A. Bell (CSO), Thomas Geballe, Thomas Giesen, Thomas G. Phillips (CSO)","submitted_at":"2010-05-31T10:26:31Z","abstract_excerpt":"We report the detection of absorption lines by the reactive ions OH+, H2O+ and H3O+ along the line of sight to the submillimeter continuum source G10.6$-$0.4 (W31C). We used the Herschel HIFI instrument in dual beam switch mode to observe the ground state rotational transitions of OH+ at 971 GHz, H2O+ at 1115 and 607 GHz, and H3O+ at 984 GHz. The resultant spectra show deep absorption over a broad velocity range that originates in the interstellar matter along the line of sight to G10.6$-$0.4 as well as in the molecular gas directly associated with that source. 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