A 16 Millisecond X-Ray Pulsar in the Crab-Like SNR N157B: Fast Times at   30 Doradus
  The supernova remnant N157B (30 Dor B, SNR 0539-69.1, NGC 2060), located in the Tarantula Nebula of the Large Magellanic Cloud, has long been considered a possible Crab-like remnant. This hypothesis has been confirmed, quite spectacularly, with the discovery of PSR J0537-6910, the remarkable 16 ms X-ray pulsar in N157B. PSR J0537-6910 is the most rapidly spinning pulsar found to be associated with a supernova remnant. Here we report our discovery and summarize the properties of this pulsar and its supernova remnant. 
E. V. Gotthelf, W. Zhang, F. E. Marshall (GSFC/NASA), J. Middleditch   (LANL), Q. D. Wang (NWU)