Future X-ray missions employing this technology will provide vastly improved absorption - and emissionline spectroscopy of high - energy astrophysical sources such
as black hole winds and hot gas in the cosmic web.
Not exact matches
The team interpreted those shifts
as the effect of cyclonic
winds moving above and below the
black hole at speeds of about 4000 kilometers per second, tens of thousands of times stronger than the most intense cyclones on Earth.
Previously, astronomers have used x-ray telescopes to observe strong
winds very near the massive
black holes at galactic centers (artist's concept, inset) and infrared wavelengths to detect the vast outflows of cool gas (bluish haze in artist's concept, main image) from such galaxies
as a whole, but they've never done so in the same galaxy.
Astronomers have observed tornadolike
winds powered by a central active supermassive
black hole, such
as the one in this image, pervading a galaxy.
Big stars with low metal content don't shed
as much of their mass over time, so when one of them dies, almost all of its mass will
wind up in the
black hole.
«At a certain point the
black hole becomes so big
as to develop an «energetic
wind», which sweeps away gas and dust from its surrounding environment.
As a swirling disk of gas gradually falls into the central
black hole, it heats up and some of the gas is blown off the disk by intense radiation in a
wind at speeds up to a tenth of light speed (more illustrations).