NGC 2359, NGC 6888, and Wolf-Rayet Stars.

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Abstract

Radio observations give the fluxes of the two shell nebulae, and, for NGC 2359, the radio spectrum, which is flat, or thermal The shells appear to surround Wolf-Rayet stars whose distances can be estimated. Various optical data are combined with the radio data to model NGC 6888 as a shell formed by ejection of matter from the star against the interstellar gas, and to suggest the same occurrence in NGC 2359.

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