Wickramasinghe, N. C. ; Edmunds, M. G. ; Chitre, S. M. ; Narlikar, J. V. ; Ramadurai, S. (1975) A dust model for the cosmic microwave background Astrophysics and Space Science, 35 (1). L9-L13. ISSN 0004-640X
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Official URL: http://www.springerlink.com/content/pm1h27251287jh...
Related URL: http://dx.doi.org/10.1007/BF00644839
Abstract
The cosmic microwave background may be explained on the basis of absorption and reemission of the light from galaxies by graphite whiskers of lengths l⋍0.1-1 mm. The mass density of such particles required is of the order of 10−34 g cm−3.
| Item Type: | Article |
|---|---|
| Source: | Copyright of this article belongs to Springer. |
| ID Code: | 41213 |
| Deposited On: | 27 May 2011 06:56 |
| Last Modified: | 05 Jun 2011 04:51 |
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