A Tour of IGR J11014-6103
Narrator (April Hobart, CXC): Astronomers have found a remarkable object in our Milky Way galaxy. This object is a pulsar, the spinning dense core that remains after a massive star has exploded and collapsed. When this pulsar was created, something interesting happened because this pulsar is racing away from the supernova remnant where it was born at a speed between 2.5 million and 5 million miles per hour. This supersonic pace makes this pulsar - called IGR J1104-6103 -- one of the fastest moving pulsars ever observed. And what's more is that this runaway pulsar is leaving behind an extraordinary tail behind it as it goes. This tail is about 37 light years in length, making it the longest X-ray jet ever seen from an object in the Milky Way galaxy. New data from NASA's Chandra X-ray Observatory have been combined with radio data from the Australia Telescope Compact Array to provide astronomers with a more complete picture of what's happening in this system. For example, these data show that the tail has a distinct corkscrew shape. This suggests that the pulsar is wobbling like a top as it spins. IGR J1104-6103 is located about 60 light years away from the center of the supernova remnant SNR MSH 11-61A, which is where astronomers think the pulsar was originally created. By examining the details of the pulsar, its jet, and the supernova remnant, astronomers are piecing together the story of this exceptional object in our Galaxy.
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