The isotopic abundance of interstellar oxygen derived from 18-cm line observations

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Astronomical Spectroscopy, Interstellar Gas, Molecular Clouds, Molecular Rotation, Oxygen Isotopes, Abundance, Hydroxyl Radicals, Line Spectra, Molecular Energy Levels

Scientific paper

The authors report the observation of 18OH absorption in a cold cloud located near the galactic center, and in another one close to the sun. The 16OH/18OH ratio in these sources is found higher than the ratios previously derived in hot sources and equal, within the rather large errors, to the terrestrial 16O/18O ratio. Due to their low abundance, 18OH and 17OH are unlikely to be anomalously excited, and their 18-cm opacity ratio is expected to be equal to their column density ratio. The authors' observations of 18OH and 17OH in Sgr B2 yield an abundance ratio of 3.6±0.5, similar to the C18O/C17O and HC18O+/HC17O+ ratios and 1.5 times smaller than the terrestrial 18O/17O abundance ratio.

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