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The analysis of radial velocities of interstellar spectral features: CH,CH$^{+}$ as well as 4964 and 6196 diffuse interstellar bands, seen in spectraof HD 151932 and 152233, suggests that carrier of the former is spatiallycorrelated with CH while that of the latter -- with CH$^{+}$. A furtheranalysis, done in this paper and based on the sample of 106 reddened OB stars,partly confirms this suggestion, showing that the CH column density correlatesindeed much better with the equivalent width of the 4964 DIB than with that ofthe 6196 DIB. However, the strengths of the 6196 DIB correlate only marginallybetter with CH$^+$ than with CH.

Carriers of 4964 and 6196 diffuse interstellar bands and environments dominated by either CH or CH$^{+}$ molecules