Candidate red supergiants from Gaia DR3 BPRP spectra: From the Perseus to the Scutum-Crux spiral arms

Open Access

Fig. 3

Left panel: estimated A_{K_s} (tot) values versus 3D dust map A_{K_s} (Bay 19) values. Center panel: A_{K_s} (tot)-A_{K_s} (env) values versus 3D dust map A_{K_s} (Bay 19) values. Right panel: for 16 stars with T_eff < 3600 K and τ_2.2 > 0.1, the A_{K_s} (tot) −A_{K_s} (env) values versus A_{K_s} (Mes24) values are plotted.

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