Microwave detection of interstellar HDO
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Abstract
view Abstract Citations (50) References (24) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Microwave detection of interstellar HDO. Turner, B. E. ; Zuckerman, B. ; Fourikis, N. ; Morris, M. ; Palmer, P. Abstract Results are reported for observations of the 1(11)-1(10) transition of HDO in emissions at a wavelength of 3.72 mm toward the Kleinman-Low nebula (KL) in Orion A. A preliminary abundance ratio of deuterated to nondeuterated water is calculated, and possible excitation mechanisms are considered for the detected HDO transition. Analysis indicates that the present transition has a population inversion for a wide range of kinetic temperatures, total particle densities, and projected densities of HDO, and that the HDO line probably represents thermal or quasi-thermal emission from interstellar water molecules. It is concluded that most of the oxygen in KL is probably contained in water molecules provided the ratio of deuterated water to nondeuterated water is about equal to the ratio of D to H. Publication: The Astrophysical Journal Pub Date: June 1975 DOI: 10.1086/181828 Bibcode: 1975ApJ...198L.125T Keywords: Abundance; Deuterium; Interstellar Matter; Microwave Emission; Nebulae; Electron Transitions; Fractionation; Interstellar Radiation; Masers; Molecular Energy Levels; Molecular Excitation; Population Inversion; Radial Velocity; Spectral Emission; Spectrum Analysis; Astrophysics full text sources ADS |
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