Gravitational lens helps Chandra find rare type of Black Hole | 5/11/1999 | ||||||
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The left hand panel shows the Chandra X-ray Observatory image of a powerful point-like source of X rays. The Hubble Space Telescope image (right panel) shows the spiral galaxy with which the X-ray source is associated. The X-ray source is located at the center of the galaxy, and has a deficit of low energy X rays, consistent with absorption by a thick cloud of gas. | ||||||
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Image Credit: X-ray: NASA/IOA/Fabian et al., Optical: NASA/U.Durham/Smail et al. | |||||||
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The
left hand panel shows the Chandra X-ray Observatory image of a powerful
point-like source of X rays. The Hubble Space Telescope image (right panel)
shows the spiral galaxy with which the X-ray source is associated. The X-ray
source is located at the center of the galaxy, and has a deficit of low
energy X rays, consistent with absorption by a thick cloud of gas. The combination
of powerful X-ray emission, absorption of low energy X-rays, and the relatively
normal optical appearance of the galaxy suggests that the source is a rare
type of black hole called a Type 2 quasar.
The spread-out appearance of the X-ray source is an instrumental artifact. The distribution of X rays is consistent with this source being point-like. The X-ray and optical image panels have the same scale, which is 10 arcsec on a side. |
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A
team of astronomers from England and France have reported strong evidence
for the existence of a rare type of black hole, called a Type 2 quasar.
Using NASA's Chandra X-ray Observatory, they have discovered a powerful
source of X rays that appears to be a giant black hole that is hidden from
optical telescopes by a veil of obscuring material.
Type 2 quasars have been predicted to exist by a popular model for quasars. Their discovery would confirm the so-called unified model for quasars, and help clarify the nature of the pervasive background glow at X-ray and submillimeter energies. Evidence for Type 2 quasars has been reported by other researchers, but the data were ambiguous. Now, the cloud of uncertainty is lifting, as scientists use Chandra to intensify the search. According to the unified model of quasars, a thick doughnut of gas and dust surrounds a central black hole. The source looks different, depending on whether it is observed through the doughnut, through the hole, or at an intermediate angle. In extreme cases representing a Type 2 quasar, the optical radiation from the quasar is absorbed while the high energy X rays penetrate the veil. The energy absorbed by the gas and dust is re-radiated at lower energy infrared and submillimeter wavelengths. |
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