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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/2746

Title: On the morphology of supernova remnants
Authors: Radhakrishnan, V.
Srinivasan, G.
Issue Date: 1981
Citation: Advances in Space Research, 1981, Vol.1, p95-98
Abstract: The 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.
Description: Restricted Access.
URI: http://hdl.handle.net/2289/2746
ISSN: 0273-1177
Alternative Location: http://adsabs.harvard.edu/cgi-bin/bib_query?1981AdSpR...1...95R
http://dx.doi.org/10.1016/0273-1177(81)90179-4
Copyright: 1981 Elsevier B.V.
Appears in Collections:Research Papers (A&A)

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