Publication Abstracts

Herbst et al. 1977

Herbst, E., S. Green, P. Thaddeus, and W. Klemperer, 1977: Indirect observation of unobservable interstellar molecules. Astrophys. J., 215, 503-510, doi:10.1086/155381.

It is suggested that the abundances of neutral nonpolar interstellar molecules unobservable by radioastronomy can be systematically determined by radio observations of the protonated ions. As an example, observed N2H+ column densities are analyzed to infer molecular nitrogen abundances in dense interstellar clouds. The chemistries and expected densities of the protonated ions of O2, C2, CO2, C2H2, and CH4 are then discussed. Microwave transition frequencies for HCO2+ and C2H3+ are estimated, and a preliminary astronomical search for HCO2+ is described.

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BibTeX Citation

  author={Herbst, E. and Green, S. and Thaddeus, P. and Klemperer, W.},
  title={Indirect observation of unobservable interstellar molecules},
  journal={Astrophysical Journal},

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RIS Citation

ID  - he03000u
AU  - Herbst, E.
AU  - Green, S.
AU  - Thaddeus, P.
AU  - Klemperer, W.
PY  - 1977
TI  - Indirect observation of unobservable interstellar molecules
JA  - Astrophys. J.
JO  - Astrophysical Journal
VL  - 215
SP  - 503
EP  - 510
DO  - 10.1086/155381
ER  -

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