This location is emitting synchrotron radiation and it is home to a slowing down pulsar.
Aharonian, Bogovalov, and Khangulyan have recently proposed a model based on cold unrelativistic wind to explain observations of this location. Kennel and Coroniti developed a magnetohydrodynamic model to explain the boundaries of this place. Its internal structure includes a torus at a right angle to its internal axis and the "inner ring." Discovered by John Bevis, this is the brightest gamma ray source in the heavens. This location is emitting synchrotron radiation and it is home to a slowing down pulsar. This object is believed to be the remnants of a supernova in 1054. For 10 points, name this nebula that is M1 in the Messier Catalog.
Aharonian, Bogovalov, and Khangulyan have recently proposed a model based on cold unrelativistic wind to explain observations of this location.
Crab Nebula [or M1 before mentioned; or Crab Pulsar]