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Fig. 4

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Relationship between the extinction-normalized 862 nm DIB and the Schlafly et al. (2016) total to selective extinction R′V for APOGEE LOSs (dots). For low to moderate extinctions, despite the large scatter, DIBnorm 862$\[\mathrm{DIB}_{\text {norm }}^{862}\]$ decreases with RV1$\[R_V^{\prime-1}\]$. To illustrate the trend, iso-contours of data point numbers per 0.007 × 0.04 rectangular bins in RV1$\[R_V^{\prime-1}\]$ × DIBnorm 862$\[\mathrm{DIB}_{\text {norm }}^{862}\]$ are drawn for 40, 80, and 120 points. The trend is reversed at very high extinctions, as shown by the superimposed results of Ramírez-Tannus et al. (2018) for M17 (thick crosses). For these data points we neglected the difference between R′V and RV. All markers are colour-coded according to the LOS extinction.

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