Fig. 10 from Gas‐Phase Electronic Spectra of Carbon‐Chain Radicals Compared with Diffuse Interstellar Band Observations

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

Gas‐Phase Electronic Spectra of Carbon‐Chain Radicals Compared with Diffuse Interstellar Band Observations

Authors: T. Motylewski, H. Linnartz, O. Vaizert, J. P. Maier, G. A. Galazutdinov, F. A. Musaev, J. Krełowski, G. A. H. Walker, and D. A. Bohlender

Motylewski et al. 2000 The Astrophysical Journal 531 312.

Provider: AAS Journals

Caption: Fig. 10.

Origin band of the ﹩^{2}\Pi \leftarrow X^{2}\Pi ﹩ electronic transition of HC﹩_{5}﹩N﹩^{+}﹩ in the gas phase (bottom) compared to three selected stars. The C IV feature blends a possible DIB. The astronomical spectra show a weak interstellar feature coinciding with the laboratory spectrum.

Other Images in This Article

Copyright and Terms & Conditions