Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/2746
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dc.contributor.authorRadhakrishnan, V.-
dc.contributor.authorSrinivasan, G.-
dc.date.accessioned2007-06-11T11:13:47Z-
dc.date.available2007-06-11T11:13:47Z-
dc.date.issued1981-
dc.identifier.citationAdvances in Space Research, 1981, Vol.1, p95-98en
dc.identifier.issn0273-1177-
dc.identifier.urihttp://hdl.handle.net/2289/2746-
dc.descriptionRestricted Access.en
dc.description.abstractThe difference in morphology between filled and shell type supernova remnants is attributed to differences in the activity of the neutron stars left by the supernovae. Pulsar activity leads to centrally concentrated remnants similar to the Crab. Non-activity as a pulsar results in all of the rotational energy loss going into dipole radiation. The pressure of this radiation creates shell-like objects with hollow interiors such as Cas A.en
dc.format.extent197407 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.relation.urihttp://adsabs.harvard.edu/cgi-bin/bib_query?1981AdSpR...1...95Ren
dc.relation.urihttp://dx.doi.org/10.1016/0273-1177(81)90179-4en
dc.rights1981 Elsevier B.V.en
dc.titleOn the morphology of supernova remnantsen
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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