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Black Holes In Feeding Frenzy
Honolulu, HI (SPX) Aug 06, 2007 Two UH astronomers using the Hubble Space Telescope believe they have identified what makes at least some quasars shine: the black hole at the center of a massive galaxy with little gas of its own is gobbling up material from a colliding gas-rich galaxy. The merging of two galaxies has long been thought to be an efficient way of driving gas deeply into a galaxy to feed the central black hole, but there was only indirect evidence for such a mechanism until now. It was already known that quasars, which are among the most powerful objects in the Universe, lie at the centers of giant galaxies and consist of a massive black hole surrounded by a vortex of gas. Before the gas falls into the black hole, it spins faster and faster, and its temperature rises until it is hot enough to radiate up to a trillion times the power from the Sun. The question that graduate student Hai Fu and astronomer Alan Stockton tried to answer is, "Where is the gas coming from?" To answer the question, Fu and Stockton used a telescope-mounted spectroscope to find out what the gas is made of. "We found that the gas that is spiraling into the black hole is almost pure hydrogen and helium, whereas the stars and other material in the surrounding giant galaxy are heavily contaminated by other elements such as carbon and oxygen," said Fu. This difference implies that the infalling gas has recently come from outside the galaxy, most likely from another galaxy that is merging with the giant one. Fu and Stockton also see a chaotic distribution of fast-moving patches of relatively pure hydrogen and helium scattered around the quasar, implying that black holes not only swallow things, but can also expel a large portion of their meal out to thousands of light-years away, likely through an energetic blast that happened millions of years ago. Fu and Stockton did their research at the UH Institute for Astronomy in Manoa valley using data from the Hubble Space Telescope, which is in orbit around Earth, and from the telescopes on Mauna Kea, the Big Island. Their work has been published in the August 1 issue of the Astrophysical Journal Letters. Related Links Institute for Astronomy, University of Hawaii at Manoa Understanding Time and Space
Chandra Catches Piranha Black Holes
Cambridge, MA (SPX) Jul 25, 2007Supermassive black holes have been discovered to grow more rapidly in young galaxy clusters, according to new results from NASA's Chandra X-ray Observatory. These "fast-track" supermassive black holes can have a big influence on the galaxies and clusters that they live in. Using Chandra, scientists surveyed a sample of clusters and counted the fraction of galaxies with rapidly growing supermassive black holes, known as active galactic nuclei (or AGN). The data show, for the first time, that younger, more distant galaxy clusters contained far more AGN than older, nearby ones. |
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