The smaller member of the Cygnus X-1 binary star system is thought to be one of these objects evidenced by its mass being too large for a neutron star.
The smaller member of the Cygnus X-1 binary star system is thought to be one of these objects evidenced by its mass being too large for a neutron star. Rotating variations have a ring-like center and a region (*) called the ergosphere where it becomes impossible to remain stationary. The Schwarzchild radius is the distance from the central singularity to the event horizon of, FTP, these astronomical objects that possess such a massive escape velocity that light cannot escape their gravitational pull.
The smaller member of the Cygnus X-1 binary star system is thought to be one of these objects evidenced by its mass being too large for a neutron star.
Black Holes