An efficient gas phase synthesis for interstellar PN

Details An efficient gas phase synthesis for interstellar PN An efficient gas phase synthesis for interstellar PN

Dec 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987mnras.229p..41m&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 229, Dec. 1, 1987, p. 41P-44P.

Other

19

Interstellar Chemistry, Molecular Clouds, Nitrides, Phosphorus Compounds, Synthesis (Chemistry), Vapor Phases, Abundance, Astronomical Models, Time Dependence

Scientific paper

Previous models of phosphorus chemistry in dense interstellar clouds are extended to include a gas phase systhesis for the newly observed interstellar molecule, PN (phosphorus nitride). A time-dependent calculation shows that the abundance of PN and upper limits to the abundances of other phosphorus-bearing molecules are reproduced without the need to invoke grain disruption or high-temperature reactions.

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