Herschel/HIFI discovery of interstellar chloronium (H2Cl +)

Abstract

We report the first detection of chloronium, H2Cl+, in the interstellar medium, using the HIFI instrument aboard the Herschel Space Observatory. The 212-101 lines of ortho-H235Cl+ and ortho-H237Cl+ are detected in absorption towards NGC 6334I, and the 111-0 00 transition of para-H235Cl+ is detected in absorption towards NGC 6334I and Sgr B2(S). The H2Cl + column densities are compared to those of the chemically-related species HCl. The derived HCl/H2Cl+ column density ratios, ∼1-10, are within the range predicted by models of diffuse and dense photon dominated regions (PDRs). However, the observed H2Cl+ column densities, in excess of 1013 cm-2, are significantly higher than the model predictions. Our observations demonstrate the outstanding spectroscopic capabilities of HIFI for detecting new interstellar molecules and providing key constraints for astrochemical models. © 2010 ESO.