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Fig. 5
Left: spectra of CH3CCH J = 5− 4, K = 0,1,2. Middle: rotation temperature diagram of CH3CCH. Right: SED of the L1489 IRS from the PACS 160 μm and SPIRE wavelengths of Herschel as well as SCUBA 850 μm. The filled squares represent the input fluxes. The line shows the best fitting of the gray-body model.
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