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XTE J1550-564 Chandra Image
Credit: Left: X-ray (NASA/CXC); Right: Illustration (CXC/M.Weiss)


Escape from the Black Hole

Black holes not only swallow matter, they can also eject matter. If a black hole is surrounded by a ring of swirling material (called an accretion disk), some of the material gets swallowed while some may get propelled in fast moving jets off the disk. These jets seem to be a characteristic of accreting black holes, though how the jets are formed is not precisely known. Mega-massive black holes at the centers of galaxies show such jets, which often stretch for millions of light years. On smaller scales, stellar-sized black holes show the same type of jet phenomena, due (astronomers believe) to the same physical mechanism as in their much larger cousins. These smaller black holes provide a laboratory for jet physics, since they evolve rapidly so that astronomers can study in detail how the jets are formed and how they fade away. The image above is a set of Chandra X-ray Observatory images of X-ray emission from XTEJ1550-564, a binary star composed of a "normal" star with a black hole companion. In 1998 the star underwent an X-ray explosion detected by the RXTE satellite, and this explosion apparently produced (or at least lit up) jets of material speeding away from the star at about half the speed of light. The Chandra image at the top left shows X-rays from the black hole at the center of the image and an X-ray bright spot marking the tip of the jet to the left of the star. In the image below that, the counter jet to the right of the star has appeared bright in X-rays, while the jet on the left shows clear motion away from the star. Finally the last image at the lower left shows that the X-ray emission from the left jet faded, while the jet on the right remained bright. The image on the right is an artist's representation of XTEJ1550-564 showing the normal star feeding the accretion disk around the black hole.


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Page Author: Dr. Michael F. Corcoran
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