Dust model for the cosmic microwave background

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dc.contributor.authorNarlikar, J. V.
dc.contributor.authorEdmunds, M. G.
dc.contributor.authorWickramasinghe, N. C.
dc.contributor.authoret al.
dc.date.accessioned2012-03-09T13:17:25Z
dc.date.available2012-03-09T13:17:25Z
dc.date.issued1975-02-07
dc.description.abstractThe 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 .en_US
dc.identifier.urihttp://hdl.handle.net/11007/1120
dc.language.isoenen_US
dc.publisherKluwer Academic Publishersen_US
dc.relation.ispartofseriesAstrophysics and Space Science;Vol. 35, 1975
dc.subjectDusten_US
dc.subjectCosmic microwaveen_US
dc.titleDust model for the cosmic microwave backgrounden_US
dc.typeArticleen_US

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