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Microwave Detection of Interstellar Formamide
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1971
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Cosmic AbundanceMicrowave SpectroscopyPhotometryEngineeringPhysicsAstrochemistryView Abstract CitationsAstrophysical PlasmaMicrowave DetectionMicrowave MeasurementMicrowave DiagnosticsRadio TelescopeHyperfine ComponentsSpace WeatherHigh-energy AstrophysicsInterstellar Formamide Rubin
view Abstract Citations (149) References (10) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Microwave Detection of Interstellar Formamide Rubin, R. H. ; Swenson, G. W., Jr. ; Benson, R. C. ; Tigelaar, H. L. ; Flygare, W. H. Abstract Formamide was detected by its microwave emission from the 2 H 202 rotational transition at 4620 MHz in the direction of Sgr B2 and possibly Sgr A. There is evidence that all three of the AF = 0 hyperfine components are present. The astronomical rest frequencies are in good agreement with laboratory measurements. Publication: The Astrophysical Journal Pub Date: October 1971 DOI: 10.1086/180810 Bibcode: 1971ApJ...169L..39R full text sources ADS |