Fig. 9
H2O maser emissions distribution toward NML Cyg from VLA observation on 2008 December 20. All offsets are relative to the strongest maser emission at VLSR of −22.25 km s-1. All the maser spots are marked with circles, with sizes proportional to the logarithm of their flux densities. The position of the central star is indicated by a star. (This figure is available in color in electronic form.)
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