Doppler Broadening of Diffuse Interstellar Bands

Physics

Scientific paper

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Scientific paper

For few dozens of hot reddened stars we have measured half widths (HW) and equivalent widths (EW) of the interstellar sodium D2 line and of the narrow and relatively strong diffuse interstellar band at 6196 Å. We have searched for mutual correlations between intensities of the both lines and we found that the width of the considered diffuse band does not follow the corresponding width for D2 line.

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