This poetic name belongs to a nearby star and small black hole, or binary system, locked in mutual orbit in our galaxy.
For some time now, GRO J1655-40's black hole, which has seven times the mass of our sun, has been sucking superhot gas from the atmosphere of its companion star.
Via the Chandra satellite, Miller and his colleagues observed a wind of electrically charged particles emanating from GRO J1655-40.
The team believes the wind is produced by the same magnetic field that funnels matter into the black hole.
Other possible causes, such as heat or radiation pressure, are too weak to produce such a mighty wind, the team's data suggest.
The magnetic field itself would explain why the orbit of the disk around GRO J1655-40's black hole decays.
"Magnetic fields are going to cause friction in that gas, and that will [overcome angular momentum and] cause the gas to slowly spiral inward to the black hole," Miller said.
The researchers say such friction also explains another phenomenon: why black holes actively absorbing stellar gas can be the brightest x-ray objects in the universe.
Friction causes the disks of stellar gas surrounding black holes to superheat and glow, Miller says.
"It [can be] so bright in x-rays that its output begins to rival the summed x-ray emission of the entire rest of the Milky Way," he said.
Daniel Proga, an assistant professor of physics at the University of Nevada, Las Vegas, says the magnetic-wind argument relies mostly on indirect evidence, and not every scientist will find it convincing.
"But this is the best that can be done at the moment," Proga wrote in an accompanying Nature news article.
"Many astronomers will be motivated by such work to develop and explore this promising model," he continued.
Study co-author Miller says the fine resolution of NASA's Chandra X-ray Observatory, launched in 1999, enabled his team to collect the data for their revolutionary theory.
"Without the instrumental advances that have been realized on Chandra, work of this kind would really be impossible," he said.
The astrophysicist says a planned NASA x-ray satellite, called Constellation X, will enable similar scientific discoveries in the future.
"It will allow us to do a lot of this really very detailed work [on] far more distant black holes."
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