A reanalysis of interstellar OH absorption observations

Details A reanalysis of interstellar OH absorption observations A reanalysis of interstellar OH absorption observations

Apr 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996mnras.279l..37r&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 279, Issue 3, pp. L37-L40.

Astronomy and Astrophysics

Astronomy

14

Molecular Data, Ism: Abundances, Ism: Molecules, Ultraviolet: Interstellar

Scientific paper

We reconsider the rotational analysis of the absorption electronic A-X and D-X band systems of OH and show that interstellar observations of OH in front of bright stars have been interpreted with oscillator strengths that are too small by a factor of 2. However, the column densities reported from the various observations are approximately right, as a result of the neglect, in their interpretation, of the two different initial levels, which compensates the previous error.

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