Galactochemistry - Part Two - Interstellar Deuterium Chemistry

Details Galactochemistry - Part Two - Interstellar Deuterium Chemistry Galactochemistry - Part Two - Interstellar Deuterium Chemistry

Nov 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986mnras.223..429b&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Vol. 223, NO.2/NOV15, P. 429, 1986

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19

Scientific paper

The galactochemical model described in the preceding paper is extended to include deuterium chemistry. The results account satisfactorily for a variety of observations of enhanced abundances of some deuterium-containing molecules and ions and provide additional support for a galactic D/H ratio of 0.7 - 1.5×10-5. On the assumption that the Milky Way is a chemically typical galaxy, the cosmological implication is that the Universe is 'open'.

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