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- W2091298978 abstract "view Abstract Citations (5) References Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Possible Recombination Lines from Molecular-Hydrogen Regions Salpeter, E. E. ; Malone, R. C. Abstract Formulae are given for the expected intensities of radio recombination lines from very dense inter- stellar clouds in H I regions. Although most of the neutral hydrogen is molecular, the strongest lines should come from fl+* For the weaker lines from 112+ and H3+, the line splitting due to quadrupole effects is calculated, but is found not to widen the narrow lines (<1 km sec') appreciably. Intensities depend sensitively on the flux of ionizing radiation Publication: The Astrophysical Journal Pub Date: July 1971 DOI: 10.1086/151001 Bibcode: 1971ApJ...167...27S full text sources ADS |" @default.
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- W2091298978 date "1971-07-01" @default.
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- W2091298978 title "Possible Recombination Lines from Molecular-Hydrogen Regions" @default.
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