In this talk, Yale University's Meg Urry will first give several alternative descriptions of what a black hole is, then explain how recent multiwavelength surveys have allowed astronomers to take a census of
black hole growth across cosmic time.
Not exact matches
Decades from now new generations of space telescopes could capture the mergers of supermassive
black holes and glimpse pulsars spiraling to doom down their maws, or see snapping «cosmic strings,» proton - thin intergalactic defects in spacetime that may have been stretched
across the infant universe during an inflationary
growth spurt.
To measure the mass and
growth rate of these galaxies» active nuclei — the supermassive
black holes at the galaxies» centers — the researchers used data from 12 different ground - based telescopes spread
across the globe to complement the data from the Swift satellite.
Urry will conclude with the big picture: the evolution of the universe over the last 13 billion years, as indicated by computer simulations, and future prospects for observing
black hole growth and mergers
across the cosmos.