Hostname: page-component-586b7cd67f-2plfb Total loading time: 0 Render date: 2024-11-23T20:19:44.378Z Has data issue: false hasContentIssue false
  • English
  • Français

Light Scattering in Reflection Nebulae

Published online by Cambridge University Press:  25 April 2016

I. R. Shortt
I. R. Shortt*
Affiliation:
Department of Physics, University of Queensland
Get access Rights & Permissions [Opens in a new window]

Extract

Much of the information regarding the nature of solid particles in interstellar space has been gained through the study of the line-of-sight extinction of starlight and the polarization of starlight by these particles. Study of the optical properties of these particles can be extended through consideration of the scattering of stellar radiation in reflection nebulae. This type of approach requires the adoption of models for the star-nebula system, and the grain type to be considered. These models are then used in a theory which describes the scattering of light by an ensemble of small particles, as applied to dust nebulae. Results are thus obtained for the colour of the nebula as a function of distance from the illuminating star. These results can then be compared with the corresponding results of experimental broad-band photometry.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 1 , Issue 7 , April 1970 , pp. 330 - 332
Copyright
Copyright © Astronomical Society of Australia 1970

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

1 Greenberg, J. M., IAU Symp. No. 24, 291, Academic Press, London, 1966.Google Scholar
2 Wickramasinghe, N. C., MNRAS, 131, 177 (1965).CrossRefGoogle Scholar
3 Elvius, A. and Hall, J. S., Lowell Obs. Bull., No. 135, Vol. 6, No. 16 (1966).Google Scholar
4 Sobolev, V. V., Soviet Astron.-AJ, 4, 1 (1960).Google Scholar
5 Greenberg, J. M. and Roark, T. P., Astrophys. J., 147, 917 (1967).CrossRefGoogle Scholar