AGN feeding along a one-armed spiral in NGC 4593 - A study using ALMA CO(2–1) observations

Open Access

Fig. 7.

Comparison between the spiral arm widths and disc scale height as a function of radius in NGC 4593. The blue line represents the spiral arm widths, estimated from the observational data of CO(2−1) molecular gas. The red line shows the disc scale height, derived from 3D-BAROLO modelling.

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