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[en] VLBI observations have revealed that OH/H2O maser sources are the aggregations of blobes with the sizes of a few A.U., spreading over the distance of several 1017 cm. From the standpoint of masing mechanism, especially for the hydroxyl case, the author argues that the blobes correspond to proto-stars in the stage of forming an opaque core, and the aggregations correspond to proto-clusters. (Auth.)
Source
Sugimoto, D. (Tokyo Univ. (Japan)); Lamb, D.Q. (Harvard Univ., Cambridge, MA (USA). Center for Astrophysics); Schramm, D.N. (Chicago Univ., IL (USA)) (eds.); International Astronomical Union; 362 p; ISBN 90-277-1274-3; 
; 1981; p. 66-67; D. Reidel; Dordrecht, Netherlands; International Astronomical Union symposium no. 93 on fundamental problems in the theory of stellar evolution; Kyoto, Japan; 22 - 25 Jul 1980
; 1981; p. 66-67; D. Reidel; Dordrecht, Netherlands; International Astronomical Union symposium no. 93 on fundamental problems in the theory of stellar evolution; Kyoto, Japan; 22 - 25 Jul 1980