A resolved rotating disk wind from a young T Tauri star in the Bok globule CB 26

Open Access

Fig. 7

Marginal two-parameter χ² maps for model grid parameters M_*, i_disk, and derived by comparing the synthetic maps of the ¹²CO(2–1) disk models with the observations (robust deconvolution). Dashed lines indicate the parameter values for the chosen “best-fit” disk model that was then subtracted from the data.

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