Infrared colours and bolometric corrections of SiO masing stars in the inner Milky Way

Open Access

Fig. 2

Comparison of $A_{K_{s}}$ $\[A_{K_{\mathrm{s}}}\]$ (int) derived from different datasets. Left: $A_{K_{s}}$ $\[A_{K_{\mathrm{s}}}\]$ (int) values obtained from WISE data vs. those values from MSX data. Right: $A_{K_{s}}$ $\[A_{K_{\mathrm{s}}}\]$ (int) values obtained from GLIMPSE data vs. those values from WISE data.

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