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A 16 Millisecond X-Ray Pulsar in the Crab-Like SNR N157B: Fast Times at 30 Doradus

E. V. Gotthelf·W. Zhang·F. E. Marshall·J. Middleditch·Q. D. Wang
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Abstract

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.

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E. V. Gotthelf, W. Zhang, F. E. Marshall, J. Middleditch, Q. D. Wang. 1998-08-21. A 16 Millisecond X-Ray Pulsar in the Crab-Like SNR N157B: Fast Times at 30 Doradus. https://arxiv.org/abs/astro-ph/9808240

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