Discovery of a 0.42-s pulsar in the ultraluminous X-ray source NGC 7793 P13
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DOI: 10.1093/mnrasl/slw218
Abstract: NGC 7793 P13 is a variable (luminosity range ∼100) ultraluminous X-ray source proposed to host a stellar-mass black hole of less than 15 M⊙ in a binary system with orbital period of 64 d and… read more here.
Keywords: source; 7793 p13; ultraluminous ray; ngc 7793 ... See more keywords