Volume 428, Number 1, December II 2004
|Page(s)||117 - 120|
|Section||Interstellar and circumstellar matter|
|Published online||23 November 2004|
The abundance of + in diffuse clouds
National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA 22903-2475, USA e-mail: firstname.lastname@example.org
2 Institut de Radioastronomie Millimétrique, 300 rue de la Piscine, 38406 Saint-Martin-d'Hères, France
3 Chalmers Centre for Astrophysics and Space Science, Onsala Space Observatory, Chalmers University of Technology, 43992 Onsala, Sweden
Accepted: 23 August 2004
We used the Plateau de Bure Interferometer to search for λ3mm absorption lines of HOC+ from local diffuse and translucent clouds occulting compact extragalactic mm-wave continuum sources. We detected HOC+ in three directions with column densities only 70-120 times below that of the HCO+ isomer, a factor 5-50 higher than typically found in dense dark gas but comparable to recent observations of dense photon-dominated regions. The observed amounts of HOC+ N(HOC+)/N(H2) can be made in quiescent diffuse gas at thermal gas-kinetic rates if the H2O/OH ratio is of order unity, in mild violation of extant observational limits.
Key words: ISM: molecules / astrochemistry
© ESO, 2004
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