Cosmic iron whiskers: their origin, length distribution and astrophysical consequences

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dc.contributor.authorNarlikar, J. V.
dc.contributor.authorWickramasinghe, N. C.
dc.contributor.authorSachs, R.
dc.contributor.authoret al.
dc.date.accessioned2012-03-13T14:10:16Z
dc.date.available2012-03-13T14:10:16Z
dc.date.issued1997-01-20
dc.description.abstractThe idea that iron ejected from supernovae condenses in the form of slender whiskers is developed further. The formation mechanism and the resulting length distribution of the whiskers are related to several astrophysical and cosmological phenomena.en_US
dc.identifier.urihttp://hdl.handle.net/11007/1459
dc.language.isoenen_US
dc.publisherWorld Scientific Publishing Companyen_US
dc.relation.ispartofseriesInternational Journal of Modern Physics D;Vol.6, No. 2, 1997
dc.subjectSupernovae condensesen_US
dc.subjectCosmic iron whiskersen_US
dc.subjectAstrophysical consequencesen_US
dc.subjectAstrophysical and cosmological phenomenaen_US
dc.titleCosmic iron whiskers: their origin, length distribution and astrophysical consequencesen_US
dc.typeArticleen_US

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