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We confirm, using spectra from seven observatories, that the diffuse bands6196 and 6614 are very tightly correlated. However, their strength ratio is notconstant as well as profile shapes. Apparently the two interstellar features donot react in unison to the varying physical conditions of differentinterstellar clouds.

Observational analysis of the well--correlated diffuse bands: 6196 and 6614 \AA