The orbiting
motion of the accretion disk can trace the «death spiral» of its matter as it falls into the darkness of what the astrophysicists measure to be a supermassive black hole.
Not exact matches
«We think that the mean
motion resonances are acting like a rut, collecting debris from the
accretion epoch
of Charon,» says New Horizons principal investigator Alan Stern
of the Southwest Research Institute in Boulder, Colo., who also contributed to the new research.
In order to accurately model the behavior
of the
accretion disk that orbits our galaxy's supermassive black hole, the researchers used a method that tracked the
motion and path
of individual particles — rather than one that treats the
motion of plasma as a macroscopic fluid.