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Woodgate, B.E.; Kirshner, R.P.; Balon, R.J.
National Aeronautics and Space Administration, Greenbelt, Md. (USA). Goddard Space Flight Center1977
National Aeronautics and Space Administration, Greenbelt, Md. (USA). Goddard Space Flight Center1977
AbstractAbstract
[en] The one dimensional distribution of Fe 14 emission has been determined along a radius of the Cygnus Loop through the use of a tilting filter photometer. The observed emission extends at least 5 arc minutes outside the optical filaments. A simple Sedov solution model of the temperature and density distribution behind the shock agrees with the observations for parameters in reasonable agreement with X-ray maps and optical radial velocities
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Aug 1977; 13 p; NASA-TM-X--71393; X--681-77-224; Available from NTIS. PC A02/MF A01
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