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NASA satellite reveals new black hole info

WAX2002111801 - WASHINGTON, Nov. 18 (UPI) -- This is an artist's rendition of a black hole, likely created by a supernova, streaking across our galaxy while slowly consuming the companion star it has in tow. GRO J1655-40 is the second so-called 'microquasar' discovered in our Galaxy. Microquasars are black holes of about the same mass as a star. They behave as scaled-down versions of much more massive black holes that are at the cores of extremely active galaxies, called quasars. Astronomers have known about the existence of stellar-mass black holes since the early 1970s. Their masses can range from 3.5 to approximately 15 times the mass of our Sun. Using Hubble data, astronomers were able to describe the black-hole system. The companion star had apparently survived the original supernova explosion that created the black hole. It is an aging star that completes an orbit around the black hole every 2.6 days. It is being slowly devoured by the black hole. Blowtorch-like jets (shown in blue) are streaming away from the black-hole system at 90 percent of the speed of light. rlw/ESA, NASA, and Felix Mirabel UPI
WAX2002111801 - WASHINGTON, Nov. 18 (UPI) -- This is an artist's rendition of a black hole, likely created by a supernova, streaking across our galaxy while slowly consuming the companion star it has in tow. GRO J1655-40 is the second so-called 'microquasar' discovered in our Galaxy. Microquasars are black holes of about the same mass as a star. They behave as scaled-down versions of much more massive black holes that are at the cores of extremely active galaxies, called quasars. Astronomers have known about the existence of stellar-mass black holes since the early 1970s. Their masses can range from 3.5 to approximately 15 times the mass of our Sun. Using Hubble data, astronomers were able to describe the black-hole system. The companion star had apparently survived the original supernova explosion that created the black hole. It is an aging star that completes an orbit around the black hole every 2.6 days. It is being slowly devoured by the black hole. Blowtorch-like jets (shown in blue) are streaming away from the black-hole system at 90 percent of the speed of light. rlw/ESA, NASA, and Felix Mirabel UPI | License Photo

COLLEGE PARK, Md., May 26 (UPI) -- NASA says data from its Swift satellite have helped astronomers determine why only about one percent of supermassive black holes emit vast amounts of energy.

Space agency scientists said the new data confirm black holes "light up" when galaxies collide, and the findings might offer insight into the future behavior of the black hole in our own Milky Way galaxy.

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The scientists said intense emission from galaxy centers, or nuclei, arises near a supermassive black hole containing between a million and a billion times the sun's mass. Giving off as much as 10 billion times the sun's energy, some of the active galactic nuclei include quasars and blazars.

"Theorists have shown that the violence in galaxy mergers can feed a galaxy's central black hole," said Michael Koss, the study's lead author and a graduate student at the University of Maryland. "The study elegantly explains how the black holes switched on."

The research that also included Neil Gehrels, Richard Mushotzky, Sylvain Veilleux and Lisa Winter is to be reported in the June 20 issue of The Astrophysical Journal Letters.

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