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Vibrationally Excited Silicon Monoxide Masers

Published online by Cambridge University Press:  14 August 2015

D. Buhl ,
F. O. Clark ,
G. Chin ,
D. Glenar ,
T. Kostiuk ,
M. J. Mumma  and
F. J. Lovas
D. Buhl
Affiliation:
1NASA-GSFC IR and Radio Astronomy Branch, Greenbelt, MD 20771
F. O. Clark
Affiliation:
2University of Kentucky, Lexington, KY 40506
G. Chin
Affiliation:
1NASA-GSFC IR and Radio Astronomy Branch, Greenbelt, MD 20771
D. Glenar
Affiliation:
1NASA-GSFC IR and Radio Astronomy Branch, Greenbelt, MD 20771
T. Kostiuk
Affiliation:
1NASA-GSFC IR and Radio Astronomy Branch, Greenbelt, MD 20771
M. J. Mumma
Affiliation:
1NASA-GSFC IR and Radio Astronomy Branch, Greenbelt, MD 20771
F. J. Lovas
Affiliation:
3National Bureau of Standards, Washington, D.C. 20234

Abstract

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Published data on a select group of SiO maser sources have been analyzed for velocity variations as a function of phase. No apparent correlation was found to a level of about 2 km/s. This places constraints on the location of the maser molecules. Such a correlation should be present at some level. The implications for future high resolution infrared measurements are discussed.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 87: Interstellar Molecules , 1980 , pp. 537 - 538
Copyright
Copyright © Reidel 1980 

References

Hinkle, K.H.: 1978, Astrophys. J. 220, 210.CrossRefGoogle Scholar
Scalise, E., and Lepine, J.R.D.: 1978, Astron. & Astrophys. 65, L7.Google Scholar
Snyder, L.E., Buhl, D., Dickson, D., and Dickinson, A.: 1980, in preparation.Google Scholar