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Broadband Structure in the Interstellar Extinction Curve∗

Published online by Cambridge University Press:  14 August 2015

D. S. Hayes ,
G. E. Mavko ,
R. R. Radick ,
K. H. Rex  and
J. M. Greenberg
D. S. Hayes
Affiliation:
Rensselaer Polytechnic Institute, U.S.A.
G. E. Mavko
Affiliation:
Rensselaer Polytechnic Institute, U.S.A.
R. R. Radick
Affiliation:
Rensselaer Polytechnic Institute, U.S.A.
K. H. Rex
Affiliation:
Rensselaer Polytechnic Institute, U.S.A.
J. M. Greenberg
Affiliation:
State University of New York at Albany, N.Y., U.S.A.

Abstract

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We have analysed observations of the interstellar extinction in the range 3400 Å–l 1000 Å. The observations have high photometric accuracy and wavelength resolution, and allow a detailed examination of broadband structure as well as the general shape of the wavelength dependence of the extinction curve. The broadband structure has a characteristic size of several hundred ångströms, and may be as important as the diffuse bands in indicating the physical nature of the grains.

We describe our preliminary theoretical interpretation of this broadband structure, and the new observation which it predicts.

Type
Part II Diffuse Features
Information
Symposium - International Astronomical Union , Volume 52: Interstellar Dust and Related Topics , 1973 , pp. 83 - 90
Copyright
Copyright © Reidel 1973 

References

Greenberg, J. M.: 1973, in Gordon, M. A. and Snyder, L. E. (eds.), Molecules in the Galactic Environments (John Wiley and Sons), Proceedings of a Symposium on Interstellar Molecules, held at Charlottesville, Virginia, October 1971, p. 93.Google Scholar
Greenberg, J. M. and Stoeckly, R.: 1971, Nature Phys. Sci. 230, 15.Google Scholar
Harris, J. W.: 1969, Nature 223, 1046.Google Scholar
Hayes, D. S.: 1970, Astrophys. J. 159, 165.Google Scholar
Nandy, K.: 1964, Publ. Roy. Obs. Edinburgh 3, 142.Google Scholar
Oke, J. B.: 1964, Astrophys. J. 140, 689.Google Scholar
Oke, J. B. and Schild, R. E.: 1970, Astrophys. J. 161, 1015.Google Scholar
Shah, G.: 1967, Unpublished dissertation, Rensselaer Polytechnic Institute.Google Scholar
Underhill, A. B. and Walker, G. A. H.: 1966, Monthly Notices Roy. Astron. Soc. 131, 475.CrossRefGoogle Scholar
Walker, G. S. H.: 1967, Astron. J. 72, 37.Google Scholar
Whiteoak, J. B.: 1966, Astrophys. J. 144, 305.Google Scholar
Whitford, A. E.: 1958, Astron. J. 63, 201.Google Scholar
Wickramasinghe, N. C.: 1967, in Greenberg, J. M. and Roack, T. P. (eds.), Interstellar Grains , NASA SP-140, p. 37.Google Scholar
Wickramasinghe, N. C. and Guillaume, C.: 1965, Nature 207, 366.Google Scholar