Excitation temperature of C2 and broadening of the 6196A diffuse interstellar band
arXiv:1009.5192 · doi:10.1051/0004-6361/200811558
Abstract
This paper presents a finding of the correlation between the width of a strong diffuse interstellar band at 6196A and the excitation temperature of C2 based on high resolution and high signal-to-noise ratio spectra. The excitation temperature was determined from absorption lines of the Phillips A-X and Mulliken D-X systems. The width and shape of the narrow 6196A DIB profile apparently depend on the C2 temperature, being broader for higher values.
arXiv comment7 pages, 8 figures, A&A 2009
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- Abundances and rotational temperatures of the C2 interstellar molecule towards six reddened early-type stars
- Using machine learning to classify the diffuse interstellar bands
- Centrosymmetric molecules as possible carriers of diffuse interstellar bands
- The 6614 diffuse interstellar absorption band: evidence for internal excitation of the carrier
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- The well correlated DIBs at 6196, 6614 Å and their possible companions
- Broadened profiles of Diffuse Interstellar Bands
- Position displacement of diffuse interstellar bands
- On the intrinsic rest wavelengths of diffuse interstellar bands
- Survey of Profile Parameters of the Diffuse Interstellar Band. From Uniform Profiles to Doppler Splitting and Blueshifts
- The EDIBLES survey. X. The 6196 Å diffuse interstellar band: Identification of side DIBs as an indication of a small carrier molecule
- On a common carrier hypothesis for the 6613.6 and 6196.0 Å diffuse interstellar bands