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- W1561330338 abstract "We review the interferometric observations of OH masers in star-forming regions emphasising VLBI data. Using a model of the OH maser zone described in Gray et al. (1991, MNRAS, 252) and a theory of maser propagation in Field & Gray (1988, MNRAS, 234) we attempt to establish the physical conditions under which intense maser beams may form in the 18, 5 and 6 cm lines. It is shown, for example, that bright 1665 MHz spots indicate the presence of velocity shifts caused by accelerating flows of cold gas. Results of a similar nature are presented for the 1667, 1720, 1612, 6035 and 4765 MHz lines and the association of 1720 and 4765 MHz, well-known from observation, is demonstrated" @default.
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- W1561330338 date "1992-09-01" @default.
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- W1561330338 title "An analysis of intense OH maser emission in star-forming regions" @default.
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