or _Partido Comunista del Peru_ early)  Robert Duncan and Christopher Thompson first formulated the 
or _Partido Comunista del Peru_ early)  Robert Duncan and Christopher Thompson first formulated the definitive theory of these objects, which they proposed as an explanation for soft gamma repeaters. Much of the evidence for the existence of these objects was collected by Chryssa Kouveliotou from the Rossi X-ray Timing Explorer, and their surfaces are thought to be covered in fibers of compressed atoms, while Alfven heating is thought to drive their wind-aided spindown model of energy loss. Vacuum birefringence is hypothesized to occur in the vicinity of these objects, and like the larger class of objects to which they belong, their mass is subject to the Tolman-Oppenheimer-Volkoff limit. Forming when a helically stable dynamo arises during gravitational collapse, for ten points, identify these neutron stars with incredibly strong magnetic fields.
or _Partido Comunista del Peru_ early)  Robert Duncan and Christopher Thompson first formulated the definitive theory of these objects, which they proposed as an explanation for soft gamma repeaters.
{magnetar}s (do not accept or prompt on “neutron stars”)