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54. Optical emission from the Crab nebula in the continuous spectrum

Published online by Cambridge University Press:  18 July 2016

I. S. Shklovsky
I. S. Shklovsky*
Affiliation:
Sternberg Astronomical Institute, Moscow, U.S.S.R.

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Extensive progress of radio astronomical methods of investigation during recent years has totally changed our ideas about the nature of the enevelopes ejected during the outburst of super-novae and, consequently, also about the phenomenon of the outburst of the super-nova[1]. The only envelope of a super-nova, investigated in sufficient details by means of optical astronomy, is the Crab nebula (see W. Baade[2], Minkowski[3], Greenstein and Minkowski[4], Barbier[5]. All available explanations concerning the nature of the Crab nebula are based upon these investigations. They were also applied in general to envelopes of other super-novae. Considering the Crab nebula as a typical super-nova remnant let us shortly discuss these statements.

Type
Part VII: Additional Contributions
Information
Symposium - International Astronomical Union , Volume 6: Electromagnetic Phenomena in Cosmical Physics , 1958 , pp. 520 - 528
Copyright
Copyright © Cambridge University Press 1958 

References

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