Type: X-ray binary system
Total Mass: 35 solar masses
Cygnus X-1 contains two stars:
One star: 10 solar masses
Other star: 25 solar masses (potential candidate for a black hole)
Temperature:
The region emits X-rays indicating extremely high temperatures, ranging from several million degrees Kelvin.
X-ray Emission:
Variability of X-rays in intensity observed on a millisecond scale, indicating dynamic interactions in the system.
Diameter: 300 kilometers
Radius: 50 kilometers
Black Hole:
Possibility of being a black hole due to the mass of the secondary star and its interactions.
Accretion Disk:
Formed from matter drawn in from the companion star.
Heating up due to friction and gravitational effects, contributing to X-ray emission.
X-ray Jets:
Jets are ejected from the accretion disk as material is consumed by the black hole.
Potential Black Holes:
Astronomers believe that there are at least 20 known candidates for black holes, although newer research suggests this number may be higher.
Further Investigations:
Ongoing research and discoveries related to black holes and X-ray sources continue to advance our understanding of these cosmic phenomena.
Video Link:
A recommended video linked for visual enthusiasts interested in black holes and related phenomena.
Potential Black Holes and Their Characteristics