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Cygnus X-1 (abbreviated Cyg X-1) is a galactic X-ray source in the constellation Cygnus and was the first such source widely accepted to be a black hole. It was discovered in 1964 during a rocket flight and is one of the strongest X-ray sources detectable from Earth, producing a peak X-ray flux density of 2.3×10−23 W/(m2⋅Hz) (2.3×103 jansky). It remains…
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cygnus x-1 black x-ray hole star hde 226868 may disk mass object stellar compact system estimated x-rays accretion wind matter
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| Cygnus X-1 | Apparent magnitude (V) | 8.72 - 8.93 | 1.00 | infobox |
| Cygnus X-1 | B−V color index | +0.81 | 1.00 | infobox |
| Cygnus X-1 | Constellation | Cygnus | 1.00 | infobox |
| Cygnus X-1 | Declination | +35° 12′ 05.7845″ | 1.00 | infobox |
| Cygnus X-1 | Right ascension | 19h 58m 21.67574s | 1.00 | infobox |
| Cygnus X-1 | Spectral type | O9.7Iab | 1.00 | infobox |
| Cygnus X-1 | U−B color index | −0.30 | 1.00 | infobox |
| Cygnus X-1 | Variable type | Ellipsoidal variable | 1.00 | infobox |
| Cygnus X-1 | is a | high-mass X-ray binary system located about 7 | 0.90 | text |
| HDE 226868/Cygnus X-1 | instance of | The similarities between the emissions of X-ray binaries | 0.80 | text |
| active galactic nuclei suggests a common mechanism of energy generation involving a black hole | instance of | The similarities between the emissions of X-ray binaries | 0.80 | text |
| an orbiting accretion disk | instance of | The similarities between the emissions of X-ray binaries | 0.80 | text |
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