Hydroxyl Cation in Translucent Interstellar Clouds

Details Hydroxyl Cation in Translucent Interstellar Clouds Hydroxyl Cation in Translucent Interstellar Clouds

Aug 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010apj...719l..20k&link_type=abstract

The Astrophysical Journal Letters, Volume 719, Issue 1, pp. L20-L22 (2010).

Astronomy and Astrophysics

Astronomy

4

Ism: Molecules

Scientific paper

High-quality spectra acquired at the European Southern Observatory enabled us to discover a very weak spectral feature of the OH+ molecule, near 3584 Å. The species likely shares environments with another molecular ion, CH+. Its abundance is by a factor of 30 lower than that of neutral OH.
Based on observations collected at the European Organization for Astronomical Research in the Southern Hemisphere, Chile, under program ID 082.C-0566(A).

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