tidal disruption events造句

Large amplitude outbursts of super soft X-ray emission have been interpreted as tidal disruption events.
However other transient objects are frequently discovered, including nearby tidal disruption events, cataclysmic variables, and stellar flares, including several of the largest flares ever seen.
A tidal disruption event of this sort is when a star interacts with a supermassive black hole shredding the star, and in some cases creating a relativistic jet which produces bright emission of gamma ray radiation.
Since ~ 2009 it has become a community tool for observing transient and variable sources of all types including novae, supernovae, AGN, magnetars, galactic black hole and neutron stars, tidal disruption events, comets, etc . Several requests are received per day.
In September 2016, a team from the University of Science and Technology of China in Hefei, Anhui, China, announced that, using data from NASA Wide-field Infrared Survey Explorer, a stellar tidal disruption event was observed at a known black hole.
It's difficult to find tidal disruption events in a sentence. 用tidal disruption events造句挺难的

He has worked predominantly in the area of high energy astrophysics, studying explosive objects in the universe such as supernovae, gamma-ray bursts, gravitational wave transients and tidal disruption events ( stars torn apart when they approach too close to a massive black hole ).
It was first proposed in 1975 that tidal disruption events should be an inevitable consequence of black holes in galaxy nuclei, whereas later theorists concluded that the resulting flare of radiation from the accretion of the stellar debris could be a unique signpost for the presence of a dormant black hole in the center of a normal galaxy.
His most cited works include papers on the discovery of the origin of short gamma-ray bursts, the Swift satellite, Poisson statistics, observations of gamma-ray bursts at the edge of the visible universe, discovery of a relativistic tidal disruption event, and finding of two classes of active galactic nuclei in the gamma-ray band.
The mission has characterized the afterglow and origin of short GRB for the first time, determine the shape of the X-ray and optical afterglow lightcurves to great precision and with large statistics ( > 1000 GRBs ), provided a comprehensive data set of UV observation of supernova, and discovered X-ray outbursts from supernova shock breakouts and relativistically beamed tidal disruption events.