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- W2034214883 abstract "Kinematical models are presented of maser emission uniformly distributed throughout ellipsoidal shells with various orientations to the line of sight. The velocity fields consist of different combinations of outflow, rotation, or radial acceleration which may be produced by the central star. The models are intended to be a guide for analysis of complex, aspherical outflows. They do not depend on the evolutionary nature of the star, nor are they limited to interpretation of a specific molecule. The models are applied to and reasonably describe three complex maser sources of the Mira variable U Ori, the bipolar nebula OH 231.8+4.2 and the luminous star IRc2 in the Orion molecular cloud." @default.
- W2034214883 created "2016-06-24" @default.
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- W2034214883 date "1991-08-01" @default.
- W2034214883 modified "2023-09-26" @default.
- W2034214883 title "Kinematical models of maser shells formed by aspherical stellar outflows (I Orionis; OH 231.8 + 4.2; Orion-IRc2)" @default.
- W2034214883 doi "https://doi.org/10.1086/191593" @default.
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