Impact of the Galactic bar on tidal streams within the Galactic disc - The case of the tidal stream of the Hyades

Open Access

Fig. 5.

Position of the simulated stream (black points) formed in the case of top a: a barless Galaxy; middle b: of a barred MW with a pattern speed of Ω_b = 55 km s⁻¹ kpc⁻¹; bottom c: of a barred MW with a pattern speed of Ω_b = 39 km s⁻¹ kpc⁻¹. The red triangles indicate the position of the candidate members of the Hyades stream from the eDR3 sample of Jerabkova et al. (2021).

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