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Similar to how a low-density bubble of air will rise to the surface in water, the giant cavities in NGC become buoyant and move away from the black hole. To understand more about the black hole's history of eruptions, the researchers studied the details of the three pairs of cavities.
They found that the amount of energy required to create the pair of cavities closest to the black hole is lower than the energy that produced the older two pairs. However, the rate of energy production, or power, is about the same for all three pairs. This indicates that the eruption associated with the inner pair of cavities is still occurring.
Each of the three pairs of cavities is associated with a shock front, visible as sharp edges in the X-ray image.
These shock fronts, akin to sonic booms for a supersonic plane, heat the gas, preventing most of it from cooling and forming large numbers of new stars.
Close study of the shock fronts reveals that they are actually slightly broadened, or blurred, rather than being very sharp. This may be caused by turbulence in the hot gas. Assuming this is the case, the authors found a turbulent velocity - that is, the average speed of random motions of the gas - of aboutmiles per hourkilometers per hour.
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This is consistent with the predictions of theoretical models and estimates based on X-ray observations of the hot gas in other groups and clusters. A paper describing these results was published in the June 1st, issue of The Astrophysical Journal and is available online. The Smithsonian Astrophysical Observatory in Cambridge, Massachusetts, controls Chandra's science and flight operations.
Fast Facts for NGC