Anatomy of the Class I protostar L1489 IRS with NOEMA - II. A disk replenished by a massive streamer

Open Access

Fig. B.1

Maps of parameters obtained after the HFS fitting of C₂H. From top to bottom: T_obs × τ in K, velocity of the main component in km s⁻¹, FWHM of the main component in km s⁻¹, and group total opacity, τ.

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