New research led by astrophysicists at York University has revealed the fastest winds ever seen at UV wavelengths near a supermassive black hole. “We’re talking wind speeds of 20% the speed of light, which is more than 200 million kilometres an hour. That’s equivalent to a category 77 hurricane,” says Jesse Rogerson, York U. “And we have reason to believe that there are quasar winds that are even faster.”
Astronomers have known about the existence of quasar winds since the late 1960s. At least 1 in 4 quasars have them. Quasars are the discs of hot gas that form around supermassive black holes at the centre of massive galaxies – they are bigger than Earth’s orbit around the sun and hotter than the surface of the sun, generating enough light to be seen across the observable universe. “Black holes can have a mass that is billions of times larger than the sun,” says A/ Professor Patrick Hall. “But as matter spirals toward a black hole, some of it is blown away by the heat and light of the quasar. These are the winds that we are detecting.”
Rogerson and his team used data from Sloan Digital Sky Survey to identify new outflows from quasars. After spotting about 300 examples, they selected about 100 for further exploration, collecting data with the Gemini Observatory’s twin telescopes in Hawaii and Chile, in which Canada has a major share. “We not only confirmed this fastest-ever ultraviolet wind, but also discovered a new wind in the same quasar moving more slowly, at only 140 million kilometres an hour,” says Hall. “We plan to keep watching this quasar to see what happens next. Much of this research is aimed at better understanding outflows from quasars and why they happen.
“Quasar winds play an important role in galaxy formation,” says Rogerson. “When galaxies form, these winds fling material outwards and deter the creation of stars. If such winds didn’t exist or were less powerful, we would see far more stars in big galaxies than we actually do. http://www.eurekalert.org/pub_releases/2016-03/yu-yua032116.php
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