Redshifted Diffuse Interstellar Bands in Orion OB1 association
  The wavelength displacement of the Diffuse Interstellar Bands at 4502, 5705,
5780, 6284, and 7224 \AA\ with respect to the well known, narrow
atomic/molecular interstellar lines (of Ca{\sc ii} and Na{\sc i}) have been
measured in the spectra of the 2 Orion Trapezium stars HD 37022 and HD 37020,
using the HARPS\textendash N spectrograph, fed with the 3.5 m Telescopio
Nazionale Galileo, and the BOES spectrograph, fed with the 1.8m Korean
telescope. The red shift is $\sim$25 km/s for all these DIBs. We discuss the
various possible origins of this very peculiar wavelength shift in the light of
the particular physical conditions in the Orion Trapezium. The above mentioned
shift is seemingly absent in the DIBs at 6196 and 6993 \AA.
