A search for observational evidence of OH molecule photoproduction

Details A search for observational evidence of OH molecule photoproduction A search for observational evidence of OH molecule photoproduction

Sep 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995mnras.276..635s&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 276, Issue 2, pp. 635-639.

Other

3

Masers, Molecular Processes, Circumstellar Matter, Stars: Mass-Loss, Stars: Variables: Other, Radio Lines: Stars

Scientific paper

Observational evidence for OH molecule photoproduction by the interstellar UV radiation in the circumstellar envelopes of Mira variables has been searched for. A sample of Me-type Miras was observed in the main OH maser lines with the Nancay radio telescope. Two new lines were detected. The intensity of the 156.5-nm wavelength interstellar radiation is estimated by integration of the observed UV light of OB stars in common star catalogues. A statistically significant trend is found that OH Miras are illuminated by stronger UV fields than non-OH objects.

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