A 12.6-ms pulsar in Cygnus X-3
The X-ray binary Cygnus X-3 has long been suspected of containing a fast, young pulsar, but previous observations at various wavelengths have failed to provide any evidence of a signal with a periodicity of less than 4.8 h (the well-known periodicity in the X-ray and infrared wavebands which is ascr...
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Veröffentlicht in: | Nature (London) 1985-12, Vol.318 (6047), p.642-644 |
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Sprache: | eng |
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