The black holes that we can observe directly through their radiant emission are mostly in a configuration where gas swirls around the black hole in the form of an accretion disk and that accretion disk — most of the mass is going to be in an ionized form, and then some of that gas gets expelled from
the environment around the black hole, while it is still outside the black hole, it gets squirted out in the form of an outflow, a wind like the solar wind and then [a] much faster, collimated outflow called a jet.
Not exact matches
He and a number of colleagues theorize that energy streaming from hot gas
around a supermassive
black hole could compress, stir, and irradiate the surrounding
environment in a way that helps regulate the growth of the galaxy and the production of stars.
The nearly 100 percent polarization of the radio bursts is unusual, and has only been seen in radio emissions from the extreme magnetic
environments around massive
black holes, such as those at the centers of galaxies.
«The
environment around and the birth conditions for these
black holes actually puts them on a track either for rapid growth spurts, or for rather slow growth,» Natarajan says.
A mysterious object that repeatedly bursts with ultra-powerful radio waves must live in an extreme
environment — something like the one
around a supermassive
black hole.
These results, which were made possible by the high sensitivity and wideband observing capability of ALMA, will be a key to understanding the mysterious
environment around supermassive
black holes.
Scientists previously thought that
black holes grow by picking up mass from the
environment around them.