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C2 and Diffuse Interstellar Bands

Published online by Cambridge University Press:  21 February 2014

M. Kaźmierczak ,
M. Schmidt ,
T. Weselak ,
G. Galazutdinov  and
J. Krełowski
M. Kaźmierczak
Affiliation:
SRON Netherlands Institute for Space Research, Landleven 12, 9747 AD Groningen, The Netherlands, email: [email protected]
M. Schmidt
Affiliation:
Centre for Astronomy, Nicolaus Copernicus University, Gagarina 11, 87-100 Toruń, Poland
T. Weselak
Affiliation:
Nicolaus Copernicus Astronomical Centre, ul. Rabiańska 8, 87-100 Toruń, Poland
G. Galazutdinov
Affiliation:
Institute of Physics, Kazimierz Wielki University, Weyssenhoffa 11,85-072 Bydgoszcz, Poland
J. Krełowski
Affiliation:
Universidad Catolica del Norte, Av. Angamos 0610, Antofagasta, Chile
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Abstract

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C2, the simplest multicarbon molecule is a useful astronomical tool, because the analysis of its lines allows to determine the physical conditions in interstellar clouds. C2 abundances give information about the chemistry of interstellar clouds, especially on the pathway to the formation of long-chain carbon molecules, which may be connected with carriers of diffuse interstellar bands (Douglas 1977, Thorburn et al. 2003). Here we summarize all relations between C2 and diffuse interstellar bands (DIBs).

Keywords

ISM: moleculesISM: lines and bands
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S297: The Diffuse Interstellar Bands , May 2013 , pp. 121 - 124
Copyright
Copyright © International Astronomical Union 2014 

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