Diffuse interstellar bands as probes of small-scale interstellar structure
Keith T. Smith (1, 2), Martin A. Cordiner (3), Peter J. Sarre (1), ((1) The University of Nottingham, UK, (2) Royal Astronomical Society, UK,, (3) NASA Goddard Space Flight Center, USA)

TL;DR
This study uses diffuse interstellar bands to investigate small-scale structures in the interstellar medium, revealing variations over 0.25 parsecs and stability over 10 AU scales, with some unusual spectral features.
Contribution
It provides new observational evidence of small-scale interstellar structure using DIBs, including velocity shifts and stability over different spatial scales.
Findings
Significant DIB differences over 0.25 pc separation.
No DIB variation over ~10 AU in Kappa Vel.
Detection of an unusual DIB spectrum.
Abstract
We present observations which probe the small-scale structure of the interstellar medium using diffuse interstellar bands (DIBs). Towards HD 168075/6 in the Eagle Nebula, significant differences in DIB absorption are found between the two lines of sight, which are separated by 0.25 pc, and {\lambda}5797 exhibits a velocity shift. Similar data are presented for four stars in the {\mu} Sgr system. We also present a search for variations in DIB absorption towards {\kappa} Vel, where the atomic lines are known to vary on scales of ~10 AU. Observations separated by ~9 yr yielded no evidence for changes in DIB absorption strength over this scale, but do reveal an unusual DIB spectrum.
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