A binary black hole pair with an accretion disk inclined 45 degrees. One can see the concentric rings before they are accreted onto the black holes. Source: Nixon et al.
New research explains how a supermassive black hole might begin as a normal black hole, tens to hundreds of solar masses, and slowly accrete more matter, becoming more massive over time. The trick is in looking at a binary black hole system. When two galaxies collide the two supermassive black holes sink to the center of the merged galaxy and form a binary pair. The accretion disk surrounding the two black holes becomes misaligned with respect to the orbit of the binary pair. It tears and falls onto the black hole pair, allowing it to become more massive.
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© Shannon Hall for Universe Today, 2013. |Permalink |No comment |
Post tags: galaxies, supermassive black holes
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