Molecular line emission in NGC 4945, imaged with ALMA

C. Henkel; S. Mühle; G. Bendo; G. I. G. Józsa; Y. Gong; S. Viti; S. Aalto; F. Combes; S. García-Burillo; L. K. Hunt; J. Mangum; S. Martín; S. Muller; J. Ott; P. van der Werf; A. A. Malawi; H. Ismail; E. Alkhuja; H. M. Asiri; R. Aladro; F. Alves; Y. Ao; W. A. Baan; F. Costagliola; G. Fuller; J. Greene; C. M. V. Impellizzeri; F. Kamali; R. S. Klessen; R. Mauersberger; X. D. Tang; K. Tristram; M. Wang; J. S. Zhang

doi:10.1051/0004-6361/201732174

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Volume 615 (July 2018)

A&A, 615 (2018) A155

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Fig. 18

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Final parametrization: Intrinsic dispersion (see Sect. 4.6.1) as a function of galactocentric radius (this may be compared with Fig. 13). From top to bottom we show as in Fig. 15 c-C₃ H₂ (DSP), CH₃C₂H (DSP-2) and, overlapping, c-C₃H₂ (DSP-3) andH 42α (DSP-4; see Table 1).

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