Fine structure and kinematics of the ionized and molecular gas in the jet and disk around S255IR NIRS3 from high-resolution ALMA observations

Open Access

Fig. 3

Position-velocity diagrams for the C³⁴S(7–6) (left panel), SiO(8–7) (central panel), and CO(3–2) (right panel) emission generated along the path shown in Fig. 2. The intensity scale is in mJy beam⁻¹. The curves correspond to Keplerian rotation around the central mass of M sin² i = 10 M_⊙ (solid) and M sin² i = 15 M_⊙ (dashed), where i is the inclination angle.

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