An interpretation of the anomalous variation of N2H+/HCO+/SO2 in Orion - Support for ion-molecule reactions

Details An interpretation of the anomalous variation of N2H+/HCO+/SO2 in Orion - Support for ion-molecule reactions An interpretation of the anomalous variation of N2H+/HCO+/SO2 in Orion - Support for ion-molecule reactions

Feb 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977apj...212...79s&link_type=abstract

Astrophysical Journal, Part 1, vol. 212, Feb. 15, 1977, p. 79-83.

Astronomy and Astrophysics

Astronomy

20

Interstellar Matter, Microwave Emission, Molecular Ions, Radio Astronomy, Carbon Compounds, Nitrogen Compounds, Sulfur Oxides, Water

Scientific paper

An 11 m radio telescope was utilized in the considered observations. A description is given of the equipment and the observational technique used. A map is presented of HCO(+), N2H(+), and SO2 emission spectra in the direction of the center region of the Orion Nebula molecular cloud. Possible interpretations of an observed intensity anticorrelation are discussed, giving attention to a test of the ion-molecule scheme and an upper limit to the abundance of water.

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