TELESCOPE OBSERVATIONS OF THE SiO MASES

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1975

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Ohio State University

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In December of 1973, strong maser emission signals centered around a frequency near 86 243 MHz were detected from the direction of the Orion $Nebula^{1}$. After considering many other possibilities, we suggested that this unique maser emission might be comi

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$^{1}$ L. E. Snyder and D. Buhl, Astrophys. J. Lett. 189, L31 (1974). $^{2}$ J. H. Davis, C. N. Blair, H. VanTill, and P. Thaddeus, Astrophys. J. Lett. 190, L117 (1974). $^{3}$ P. Thaddeus, J. Mather, J. H. Davis, and G. N. Blair, Astrophys. J. Lett. 192, L33 (1974).""
Author Institution: NASA,, Goddard Space Flight Center; NASA,, University of Virginia,; NASA,, National Bureau of Standards

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http://hdl.handle.net/1811/9318

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Abstracts of OSU International Symposium on Molecular Spectroscopy 1970-1979