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- W1995989812 abstract "view Abstract Citations (1) References (10) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Distribution of 733-GHz para-formaldehyde line emission in the Orion nebula. Kaifu, N. ; Iguchi, T. ; Morimoto, M. Abstract The loi-Ooo transition of para-formaldehyde (72.8381 GHz) has been observed for 10 points in Ori A by the 6-rn millimeter-wave telescope at Mitaka. The emission has been found to be extended to the north direction compared with the 2-mm lines of formaldehyde; the north-south extension of the 73-GHz line emission is about 6'. The distribution of the excitation temperature of para-formaldehyde in the Orion molecular cloud is discussed. The column density of para-formaldehyde is estimated to be 2 5 x 10' cm-2. Subject headings: abundances, nebular - molecules, interstellar - Orion Nebula Publication: The Astrophysical Journal Pub Date: March 1975 DOI: 10.1086/153460 Bibcode: 1975ApJ...196..719K Keywords: Formaldehyde; Line Spectra; Microwave Emission; Nebulae; Abundance; Hydrogen Clouds; Interstellar Gas; Molecular Spectra; Radio Astronomy; Astrophysics full text sources ADS |" @default.
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- W1995989812 date "1975-03-01" @default.
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- W1995989812 title "Distribution of 73-GHz para-formaldehyde line emission in the Orion nebula" @default.
- W1995989812 doi "https://doi.org/10.1086/153460" @default.
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