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Supernova Remnants With Compact X-Ray Sources

Published online by Cambridge University Press:  04 August 2017

D. H. Clark ,
P. G. Murdin ,
R. Wood ,
R. Gilmozzi ,
I. J. Danziger  and
A. W. Furr
D. H. Clark
Affiliation:
(Rutherford-Appleton Laboratory)
P. G. Murdin
Affiliation:
(Royal Greenwich Observatory)
R. Wood
Affiliation:
(Royal Greenwich Observatory)
R. Gilmozzi*
Affiliation:
(Royal Greenwich Observatory)
I. J. Danziger
Affiliation:
(European Southern Observatory)
A. W. Furr
Affiliation:
(Astronomy Centre, University of Sussex)
*
Istituto di Astrofisica Spaziale, Frascati.

Extract

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More than 3000 radial velocity observations across the face of the Crab Nebula are used to investigate its 3-dimensional properties. In the standard model it consists of a thick hollow shell with synchrotron emission from within. We show that the thick shell is composed of bright inner and faint outer components

Type
V. Compact Objects Associated With Supernova Remnants, Pulsars and Neutron Stars
Information
Symposium - International Astronomical Union , Volume 101: Supernova Remnants and Their X-Ray Emission , 1983 , pp. 417 - 419
Copyright
Copyright © Reidel 1983