The Crab Nebula is not alone!

Details The Crab Nebula is not alone! The Crab Nebula is not alone!

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983obs...103...85w&link_type=abstract

The Observatory, vol. 103, p. 85-106 (1983)

Physics

43

Scientific paper

The Crab Nebula has been recognized for a number of years as but one member of a class of supernova remnants having similar morphology and physical properties. Recent results, however, imply that the number of observable "true" examples of the class may be quite small and that a more extensive third class of remnants, which combines both "shell" and "filled-centre" properties, exists. To give an overview, the identifying properties of all three groupings are outlined and examples are given for the small plerionic (Crab Nebula) and combination classes.

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