The new results, which came from the observatory «Chandra» and telescope «Magellan» show that the dense stellar remnants are the result of rupture of a star by a black hole, which is a thousand times more massive than our sun. This information is conclusive proof of the existence of intermediate-mass black holes, also is the first to catch a black hole that ripped apart a star.
Astronomers have suspected that globular cluster may contain intermediate-mass black holes, but conclusive evidence has not yet been.
Recall that black holes have different masses. Supermassive - several million to several billion times the mass of the Sun and black holes in binary systems of stellar origin - their mass from a few to several tens of solar masses.
Figure supermassive black hole.
The existence of intermediate-mass black holes remained in question until now.