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Formation of Comets: Constraints From the Abundance of Hydrogen Sulfide and Other Sulfur Species

Published online by Cambridge University Press:  07 August 2017

D. Despois ,
J. Crovisier ,
D. Bockelee-Morvan  and
P. Colom
D. Despois
Affiliation:
Observatoire de Bordeaux, B.P. 89, 33270 Floirac, France
J. Crovisier
Affiliation:
Observatoire de Paris, Section de Meudon, F-92195 Meudon, France
D. Bockelee-Morvan
Affiliation:
Observatoire de Paris, Section de Meudon, F-92195 Meudon, France
P. Colom
Affiliation:
Observatoire de Paris, Section de Meudon, F-92195 Meudon, France

Abstract

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Recent determinations of H2S and other sulfur compounds abundances in comets and in Orion KL bring new tests of the origin of cometary matter.

Type
Solar System
Information
Symposium - International Astronomical Union , Volume 150: Astrochemistry of Cosmic Phenomena , 1992 , pp. 459 - 460
Copyright
Copyright © Kluwer 1992 

References

REFERENCES

A'Hearn, M.F. 1992, these proceedings.Google Scholar
Allamandola, L.J. 1992, these proceedings.Google Scholar
Blake, G.A., Sutton, E.C., Masson, C.R., Phillips, T.G. 1987, Ap.J., 315, 621–645 CrossRefGoogle Scholar
Colom, P., Bockelee-Morvan, D., Crovisier, J., Despois, D., Paubert, G. 1992, these proceedings.Google Scholar
Crovisier, J., Despois, D., Bockelée-Morvan, D., Colom, P., Paubert, G. 1991, Icarus, accepted.Google Scholar
Despois, D. 1992, these proceedings.Google Scholar
Geballe, T.R. 1991, M.N.R.A.S., 251, 24p–25p.CrossRefGoogle Scholar
Guélin, M., Rist, C., Cernicharo, J. 1990, in Proc. 7th Manchester Astronomical Conference, Cambridge University Press, in press.Google Scholar
Kim, S.J., A'Hearn, M.F. 1991, Icarus, 90, 79–95.CrossRefGoogle Scholar
Millar, T.J., Herbst, E. 1990, A.A. 231, 466–472.Google Scholar
Minh, Y.C., Ziurys, L.M., Irvine, W.M., McGonagle, D. 1990, Ap.J., 360, 136–141 CrossRefGoogle Scholar
Mumma, M.J., Stern, A., Weissman, P.R. 1992, in Protostars and Planets III, Levy, E.H., Lunine, J.I. and Matthews, M.S. eds., Univ. of Arizona Press: Tucson.Google Scholar
Roettger, E.E. 1991, Ph.D. dissertation, Johns Hopkins University.Google Scholar
Turner, B.E. 1991, Ap.J., 76, 617–686.Google Scholar
Smith, R.G. 1991, M.N.R.A.S., 249, 172–176. Walmsley, C.M. 1989, in I.A.U. Symposium 135: Interstellar Dust, eds. Allamandola, L.J. and Tielens, A.G.G.M., 263-273.CrossRefGoogle Scholar
Yamamoto, T. 1985, A.A., 142, 31–36.Google Scholar
Yamamoto, T. 1991, in Comets in the Post-Halley Era, eds. Newburn, R.L. Jr., Neugebauer, M., and Rahe, J., Kluwer: Dordrecht, 361–376.CrossRefGoogle Scholar