On a common carrier hypothesis for the 6613.6 and 6196.0 Å diffuse interstellar bands
We explore via spectroscopic modeling whether the highly correlated diffuse interstellar bands at 6613.6 and 6196.0 Å might originate from a single molecule. Efforts were made to simulate the band contours of the DIBs along the three lines-of-sight, which have been observed by others at high resolut...
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Veröffentlicht in: | Astrophysics and space science 2016-09, Vol.361 (9), p.1, Article 305 |
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Sprache: | eng |
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