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Monitor Observations of the Orion SiO Maser

Published online by Cambridge University Press:  14 August 2015

Nobuharu Ukita
Nobuharu Ukita*
Affiliation:
Department of Astronomy, University of Tokyo

Extract

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Monitor observations of the SiO v=1, J=2−1 transition were made toward the Kleinman-Low infrared nebula. Observations were made from September 1976 to February 1980 with the 6 m mm-wave telescope of the Tokyo Astronomical Observatory. Data were taken with an acousto-optical spectrometer with a frequency resolution of about 50 kHz(Δv=0.17 km s−1).

Type
Session 2: Pre-Main-Sequence Evolution and Formation of Binary Stars
Information
Symposium - International Astronomical Union , Volume 93: Fundamental Problems in the Theory of Stellar Evolution , 1981 , pp. 100
Copyright
Copyright © Reidel 1981 

References

Genzel, R., Moran, J.M., Lane, A.P., Predmore, C.R., Ho, P.T., Hansen, S.S., and Reid, M.J. 1979, Astrophys. J. Letters, 231. L73.Google Scholar
Narita, S., Nakano, T., and Hayashi, C. 1970, Prog. Theor. Phys. 43, 942.CrossRefGoogle Scholar