Abstract
The 211?212 transition of acetaldehyde at 3195 ·167 MHz has been observed in emission in SgrB2 with the Parkes 64 m telescope. Comparison of the intensities of the 110---> 11 and 211--->212 emission lines suggests that both transitions may be inverted.
Cite
CITATION STYLE
APA
Fourikis, N., Sinclair, M., Robinson, B., Godfrey, P., & Brown, R. (1974). Microwave Emission of the 211?212 Rotational Transition in Interstellar Acetaldehyde. Australian Journal of Physics, 27(3), 425–430. https://doi.org/10.1071/ph740425
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