34. This phenomenon has been widely observed in radio wave lengths (Maser). See e.g.:
Moran, J.M.,
Radio observations of galactic masers, in:
Frontiers of Astrophysics, ed.
Avrett, E.H. (
Harvard U.P.,
1976). The multipole fragmentation of the maser sources observed in Astro-physical systems (see e.g.: Genzel, R., et al.: 1978, As. Ap. 66, 13 and references therein), could be originated by the fulfillment of the necessary conditions presented here and in ref. (33)).
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