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NGC 4636
279 of 370

NGC 4636

October 20, 2005
Chandra's image of the elliptical NGC 4636 shows spectacular symmetric arms, or arcs, of hot gas extending 25,000 light years into a huge cloud of multimillion-degree-Celsius gas that envelopes the galaxy. At a temperature of 10 million degrees, the arms are 30 percent hotter than the surrounding gas cloud.

The temperature jump, together with the symmetry and scale of the arms indicate that the arms are the leading edge of a galaxy-sized shock wave that is racing outward from the center of the galaxy at 700 kilometers per second. An explosion with an energy equivalent to several hundred thousand supernovas would be required to produce this effect.

This eruption could be the latest episode in a feedback cycle of violence that keeps the galaxy in a state of turmoil. The cycle starts when a hot gas cloud that envelops the stars in the galaxy cools and falls inward toward a central, massive black hole. The feeding of the black hole by the infalling gas leads to an explosion that heats the hot gaseous envelope, which then cools over a period of several million years to begin the cycle anew.


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