Not exact matches
The researchers modeled the resulting
accretion disc — an elliptical disc of stellar debris swirling around the black
hole — along with its probable speed, radius, and
rate of infall, or speed at which material falls onto the black
hole.
Meanwhile, a correlation between the
rate at which stars form in the central regions of galaxies and the amount of gas that falls into supermassive black
holes (mass
accretion rate) was known to exist, leading some scientists to suggest that the activity involved in star formation fuels the growth of black
holes.
Using NASA's super-sensitive Chandra X-ray space telescope, a team of astronomers led by Q. Daniel Wang at the University of Massachusetts Amherst has solved a long - standing mystery about why most super massive black
holes (SMBH) at the centers of galaxies have such a low
accretion rate — that is, they swallow very little of the cosmic gases available and instead act as if they are on a severe diet.
«From the available Chandra data for the source, we also concluded that the black
hole has a very low
accretion rate, and is therefore reached the end of its growth.
Panel (a) shows
accretion rate, (b) shows mass, (c) shows velocity, and (d) shows distance between the closest two black
holes.
In March, researchers from the Los Alamos National Laboratory in New Mexico used computer simulations to calculate the
rate of evolution of supermassive black
holes if their growth is fed by cold and dense
accretion streams.