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Molecular Observations of Comets: Constraints for Planetary System Formation

Published online by Cambridge University Press:  26 May 2016

Jacques Crovisier
Affiliation:
Observatoire de Paris, F-92195 Meudon, France
Nicolas Biver
Affiliation:
Observatoire de Paris, F-92195 Meudon, France
Dominique Bockelée-Morvan
Affiliation:
Observatoire de Paris, F-92195 Meudon, France
Pierre Colom
Affiliation:
Observatoire de Paris, F-92195 Meudon, France
Didier Despois
Affiliation:
Observatoire de Bordeaux, France
D. C. Lis
Affiliation:
California Institute of Technology, Pasadena, USA
Heike Rauer
Affiliation:
DRL Inst. of Space Sensor Tech. and Planet. Explor., Berlin, Germany

Abstract

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We review our knowledge of the composition of cometary volatiles in the light of recent observations of comets C/1996 B2 (Hyakutake) and C/1995 01 (Hale-Bopp) and examine how this could constrain models of planetary system formation.

Type
Part II: Progress in the theory of planet formation
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

Bockelée-Morvan, D. 1997, in Molecules in Astrophysics: Probes and Processes, van Dishoeck edt., Kluwer, p. 219.Google Scholar
Bockelée-Morvan, D., Gautier, D., Lis, D.C., et al. 1998, Icarus, 147, 162.Google Scholar
Bockelée-Morvan, D., Lis, D.C., Wink, J.E., et al. 2000, A&A, 353, 1101.Google Scholar
Ehrenfreund, P. & Schutte, W.A. 2000, in Astrochemistry, IAU Symp. 197, Minh, Y.C. & van Dishoeck, E.F. eds, ASP, p. 135.Google Scholar
Lis, D.C., Keene, J., Young, T.G., et al. 1997, Icarus, 130, 355.CrossRefGoogle Scholar
Meier, R., Owen, T.C., Jewitt, D.C., et al. 1998a, Science, 279, 1707.CrossRefGoogle Scholar
Meier, R., Owen, T.C., Matthews, H.E., et al. 1998b, Science, 279, 842.CrossRefGoogle Scholar