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Fullerenes in Circumstellar and Interstellar Environments

Published online by Cambridge University Press:  05 March 2015

Jan Cami
Jan Cami*
Affiliation:
Department of Physics & Astronomy, The University of Western Ontario, London ON N6A 3K7, Canada email: [email protected]
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Abstract

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In recent years, the fullerene species C60 (and to a lesser extent also C70) has been reported in the mid-IR spectra of various astronomical objects. Cosmic fullerenes form in the circumstellar material of evolved stars, and survive in the interstellar medium (ISM). It is not entirely clear how they form or what their excitation mechanism is.

Keywords

Astrochemistry(stars:) circumstellar matterISM: moleculesinfrared: ISM
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Highlights H16: Highlights of Astronomy , August 2012 , pp. 705 - 706
Copyright
Copyright © International Astronomical Union 2015 

References

Bernard-Salas, J., Cami, J., Peeters, E., et al. 2012, ApJ 757, 41CrossRefGoogle Scholar
Berné, O. & Tielens, A. G. G. M., 2012, PNAS 109, 401CrossRefGoogle Scholar
Boersma, C., Rubin, R. H., & Allamandola, L. J. 2012, ApJ 753, 168CrossRefGoogle Scholar
Cami, J., Bernard-Salas, J., Peeters, E., & Malek, S. E. 2010, Science 329, 1180Google Scholar
Clayton, G. C., De Marco, O., Whitney, B. A., et al. 2011, AJ 142, 54Google Scholar
Clayton, G. C., Kelly, D. M., Lacy, J. H., et al. 1995, AJ 109, 2096Google Scholar
Foing, B. H. & Ehrenfreund, P. 1994, Nature 369, 296CrossRefGoogle Scholar
García-Hernández, D. A., Iglesias-Groth, S., Acosta-Pulido, J. A., et al. 2011a, ApJ 737, L30Google Scholar
García-Hernández, D. A., Kameswara Rao, N., & Lambert, D. L. 2011b, ApJ 729, 126CrossRefGoogle Scholar
García-Hernández, D. A., Manchado, A., García-Lario, P., et al. 2010, ApJ 724, L39CrossRefGoogle Scholar
Gielen, C., Cami, J., Bouwman, J., Peeters, E., & Min, M. 2011, A&A 536, A54Google Scholar
Herbig, G. H. 2000, ApJ 542, 334Google Scholar
Kroto, H. W., Heath, J. R., Obrien, S. C., Curl, R. F., & Smalley, R. E. 1985, Nature 318, 162CrossRefGoogle Scholar
Micelotta, E., Jones, A. P., Cami, J., et al. 2012, ApJ 761, 35CrossRefGoogle Scholar
Moutou, C., Sellgren, K., Verstraete, L., & Léger, A. 1999, A&A 347, 949Google Scholar
Roberts, K. R. G., Smith, K. T., & Sarre, P. J. 2012, MNRAS 421, 3277CrossRefGoogle Scholar
Rubin, R. H., Simpson, J. P., O'Dell, C. R., et al. 2011, MNRAS 410, 1320Google Scholar
Sellgren, K., Werner, M. W., Ingalls, J. G., et al. 2010, ApJ 722, L54Google Scholar
Zhang, Y. & Kwok, S. 2011, ApJ 730, 126Google Scholar