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The PAH Hypothesis and the Extinction Curve

Published online by Cambridge University Press:  23 September 2016

A. Léger ,
L. Verstraete ,
L. D'Hendecourt ,
D. Défourneau ,
O. Dutuit ,
W. Schmidt  and
J. C. Lauer
A. Léger
Affiliation:
Groupe de Physique des Solides de l'E.N.S., Université Paris VII, Tour 23 2, place Jussieu 75251 Paris Cédex 05 - France
L. Verstraete
Affiliation:
Groupe de Physique des Solides de l'E.N.S., Université Paris VII, Tour 23 2, place Jussieu 75251 Paris Cédex 05 - France
L. D'Hendecourt
Affiliation:
Groupe de Physique des Solides de l'E.N.S., Université Paris VII, Tour 23 2, place Jussieu 75251 Paris Cédex 05 - France
D. Défourneau
Affiliation:
Groupe de Physique des Solides de l'E.N.S., Université Paris VII, Tour 23 2, place Jussieu 75251 Paris Cédex 05 - France
O. Dutuit
Affiliation:
Physico-Chimie des Rayonnements, Bâtiment 350, Université Paris XI F91405 ORSAY- France
W. Schmidt
Affiliation:
Biochemical Institute, Sieker Landstrasser 19, 2070 AHRENSBURG- FRG
J. C. Lauer
Affiliation:
Centre de Recherches Lorraine, NORSOLOR, Usine de Marienau 57612 FORBACH - France

Extract

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The Polycyclic Aromatic Hydrocarbon (PAH) hypothesis states that a mixture of free PAH molecules is an ubiquitous and abundant component of the interstellar matter. It has been first formulated by Léger and Puget (1984) on the basis of molecular stability that made PAHs good candidates for the very small grains proposed by Sellgren (1984). Then, they obtained strong, although not final, support from spectroscopy.

Type
Section II: The Overidentified Infrared Emission Features
Information
Symposium - International Astronomical Union , Volume 135: Interstellar Dust , 1989 , pp. 173 - 180
Copyright
Copyright © Kluwer 1989 

References

Allamandola, L. J., Tielens, A. G. G. M., and Barker, J. R. 1985, Ap. J. (Letters), 290, L25.Google Scholar
Allamandola, L. J. 1989, in IAU Symposium 135, Interstellar Dust, eds. Allamandola, L. J. and Tielens, A. G. G. M., (Dordrecht: Kluwer), p. 129.Google Scholar
Boulanger, F. and Pérault, M. 1988, Ap. J., 330, 964.CrossRefGoogle Scholar
Boulanger, F., Baud, B., van Albada, G. D. 1985, Astr. Ap., 144, L9.Google Scholar
Cherchneff, I., and Barker, J. 1989, in Interstellar Dust Contributed Papers, eds. Tielens, A. G. G. M. and Allamandola, L. J., NASA CP-3036.Google Scholar
Crawford, M. K., Tielens, A. G. G. M., Allamandola, L. J. 1985, Ap. J. (Letters), 293, L45.CrossRefGoogle Scholar
Donn, B. 1968, Ap. J. (Letters), 152, L129.Google Scholar
Duley, W. W. and Williams, D. A. 1981, M. N. R. A. S., 196, 269.Google Scholar
Giard, M., Pajot, F., Lamarre, J. M., Serra, G., Andouze, J., Caux, E., Combes, M., Gispert, JR., Léger, A. and Rouan, D. 1988, Astr. Ap., 201, L1.Google Scholar
Giard, M., Pajot, F., Caux, E., Lamarre, J. M., and Serra, G. 1989, in Interstellar Dust Contributed Papers, eds. Tielens, A. G. G. M. and Allamandola, L. J., NASA CP-3036.Google Scholar
Greenberg, M. and Chlewicki, G. 1983, Ap. J., 272, 563.Google Scholar
Léger, A. and d'Hendecourt, L. 1985, Astr. Ap., 146, 81.Google Scholar
Léger, A. and d'Hendecourt, L. 1987, in Polycyclic Aromatic Hydrocarbons and Astrophysics, eds. Léger, A., d'Hendecourt, L., and Boccara, N., (Dordrecht: Reidel), p. 223.CrossRefGoogle Scholar
Léger, A. and Puget, J. L. 1984, Astr. Ap., 137, L5.Google Scholar
Léger, A., Boissel, P. and d'Hendecourt, L. 1988a, Phys. Rev. Letters, 60, 921.Google Scholar
Léger, A., d'Hendecourt, L. and Défourneau, D., 1988b, Astr. Ap., in press.Google Scholar
Lillie, C. F. and Witt, A. N. 1976, Ap. J., 208, 64.Google Scholar
Mathis, J. S., Metzger, P. G. and Panagia, N. 1983, Astr. Ap., 128, 212.Google Scholar
Puget, J. L. 1988, in Comet to Cosmology, ed. Lawrence, , (Springer-Verlag), p. 118.Google Scholar
Puget, J. L., Léger, A. and Boulanger, F. 1985, Astr. Ap., 142, L19.Google Scholar
Ryter, C., Puget, J. L. and Pérault, M. 1988, Astr. Ap., 186, 312.Google Scholar
Ryter, C., and d'Hendecourt, L. 1989, in Interstellar Dust Contributed Papers, eds. Tielens, A. G. G. M. and Allamandola, L. J., NASA CP-3036.Google Scholar
Sellgren, K. 1984, Ap. J., 277, 623.Google Scholar
UV Atlas 1966, (London: Butterworths).Google Scholar
van der Zwet, G. P. and Allamandola, L. J. 1985, Astr. Ap., 146, 77.Google Scholar
Verstraete, L., Léger, A., d'Hendecourt, L., Dutuit, O., Défourneau, D. 1989, in Interstellar Dust Contributed Papers, eds. Tielens, A. G. G. M. and Allamandola, L. J., NASA CP-3036.Google Scholar