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physical object > natural object > celestial body > X-ray source > Cygnus X-1
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Cygnus X-1 comparison table
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X-ray source celestial body    A class of celestial objects whose dominant mechanism of energy dissipation is through X-ray emission. Galactic X-ray sources appear optically as starlike objects, peculiar in their ultraviolet intensity, variability (on time scales ranging from milliseconds to weeks), and spectral features. All known compact X-ray sources are members of close binary systems; a current popular model is mass accretion onto a compact object from a massive companion. (Four X-ray sources - all variable - are known to be associated with globular clusters.) The 21 known extended X-ray sources associated with clusters of galaxies seem to be clouds of hot gas trapped in the cluster's gravitational field.   
Cygnus X-120 Msun X-ray source3U 1956+35> 6 Msuni ≈ 27°An X-ray source. The visible component is the ninth-magnitude supergiant HDE 226868 (O9.7 Iab). It has rapid night-to-night variations in spectral features.2.5 kpc5.5998 dayse ≈ 0.06

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