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Caption: Fig. 8.
﹩^{12}\mathrm{CO}\,﹩ and ﹩^{13}\mathrm{CO}\,﹩ ﹩J=1{\mbox{--}} 0﹩ spectra of IRAS 19475+3119 obtained at OVRO. The dashed curve in the top panel shows an empirical fit to the shape of the core emission.
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