Abstract
Using the recently available exact computations of the scattering efficiencies of spheroidal particles numerical calculations of the extinction and polarization curves have been made for a distribution of particle sizes, shapes and orientations. The results are presented and compared with the observed interstellar extinction and polarization. Possible models for interstellar dust with nonspherical grains have been discussed.
Similar content being viewed by others
References
Asano, S.: 1979,Appl. Opt. 18, 716.
Asano, S. and Sato, M.: 1980,Appl. Opt. 19 962.
Asano, S. and Yamamoto, G.: 1975,Appl. Opt. 14, 29.
Greenberg, J. M.: 1968, B. M. Middlehurst and L. H. Aller (eds.),Nebulae and Interstellar Matter, Univ. of Chicago Press, Chicago, p. 221.
Greenberg, J. M.: 1978, in J. A. M. McDonnel (ed.),Cosmic Dust, Wiley and Sons, New York, p. 187.
Greenberg, J. M.:and Hong, S. S.: 1975, in G. B. Field and A. G. W. Cameron (eds.),Dusty Universe, Neale Watson Academic Publications, Inc., New York, p. 131.
Greenberg, J. M., Lind, Z. C., Wang, R. T., and Libelo, L. F.: 1963, in M. Kerker (ed.),Electromagnetic Scattering, Pergamon Press, London, p. 123.
Greenberg, J. M., Pedersen, N. E., and Pedersen, J. C.: 1961,J. Appl. Phys. 32, 233.
Oort, J. H. and Van de Hulst, H. C.: 1946,Bull. Astron. Inst. Neth. 376, 187.
Savage, B. D. and Mathis, J. S.: 1979,Ann. Rev. Astron. Astrophys. 17, 73.
Serkowski, K. Mathewson, D. S., and Ford, V. L.: 1975,Astrophys. J. 196, 261.
Spitzer, L.: 1978,Physical Processes in the Interstellar Medium, Wiley and Sons, New York, p. 176.
Van de Hulst, H. C.: 1949,Rech. Astr. Obs. Utrecht 11, part 2.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Vaidya, D.B., Bhatt, H.C. & Desai, J.N. Interstellar extinction and polarization by spheroidal dust grains. Astrophys Space Sci 104, 323–336 (1984). https://doi.org/10.1007/BF00650306
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00650306