ALMA spectral line and imaging survey of a low and a high mass-loss rate AGB star between 335 and 362 GHz

L. Decin; A. M. S. Richards; T. Danilovich; W. Homan; J. A. Nuth

doi:10.1051/0004-6361/201732216

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Volume 615 (July 2018)

A&A, 615 (2018) A28

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This article has an erratum: [https://doi.org/10.1051/0004-6361/201732216e]

Fig. 6

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Comparison between the continuum image of IK Tau (white contours at (1, 3, 5, 10) × 0.141 mJy beam⁻¹ (3σ_rms)) and the molecular emission of HCN(4–3) (left panel) and NaCl(26–25) (right panel) showing the co-location of the dust continuum emission and the molecular emission. The molecular emission is shown for a specific frequency not corrected for the v_LSR as given in the upper right corner of each panel.

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