Very high resolution profiles of four diffuse interstellar bands

Details Very high resolution profiles of four diffuse interstellar bands Very high resolution profiles of four diffuse interstellar bands

Oct 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003mnras.345..365g&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 345, Issue 1, pp. 365-368.

Astronomy and Astrophysics

Astronomy

8

Ism: Clouds, Ism: Molecules

Scientific paper

Ultra-high-resolution (R~ 300000) profiles of four diffuse interstellar bands (DIBs) are presented. The λλ 5797-, 5850-, 6196- and 6379-Å DIBs were observed towards the reddened supergiant HD 24398, a line of sight free of Doppler splitting; thus the observed profiles can be considered as intrinsic to the DIB carriers. Three of the profiles show substructure which supports the hypothesis of a molecular origin for these DIBs.

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