Chandra/Type 2 quasar
Credit: X-ray (left): NASA/IOA/Fabian et al. Optical (right): NASA/U.Durham/Smail et al.

A Black Hole Unveiled

Active galaxies contain supermassive central black holes. These black holes generate enormous amounts of energy making active galaxies visible almost to the edge of the universe, and they often produce huge jets which extend for thousands or millions of light years. But what is the relation between these outstanding central engines and their host galaxies? Do all galaxies contain supermassive black holes? The Milky Way is thought to contain an "inactive" supermassive black hole which we can detect because it's so close to us. Detecting such black holes in the center of more distant galaxies, where the black hole may be hidden behind the thick gas and dust in the galaxy's center, is more difficult. Since X-rays can penetrate large amounts of material, astronomers can use X-ray imaging to try to unveil hidden central black holes. An X-ray image (above left) by the Chandra X-ray Observatory of a "normal" spiral galaxy (shown in optical light above right) shows that this apparently "inactive" galaxy contains a strong central X-ray source. Astronomers believe this is the signature of the central black hole in this galaxy.

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Each week the HEASARC brings you new, exciting and beautiful images from X-ray and Gamma ray astronomy. Check back each week and be sure to check out the HEAPOW archive!

Page Author: Dr. Michael F. Corcoran
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