Diffuse interstellar band λ6614 as a distance tracer for the Perseus, Taurus, and Orion molecular clouds: Feasibility and limitations

Open Access

Fig. A.1

Violin plot distribution of EW₆₆₁₄ and $V_{{LSR}_{6614}}$ ${{\rm{V}}_{{\rm{LS}}{{\rm{R}}_{6614}}}}$ errors for hot and cool stars. The left panel shows the EW error, while the right panel presents the velocity error. The pink regions represent hot stars, and the blue regions indicate cool stars. The dashed lines represent the median and mean values for each group.

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