. If further research supports the finding, it would be the first direct evidence that black holes exist.But the researcher, Joseph Dolan of NASA's Goddard Space Flight Center, cautioned that the small amount of data used in the study could contain a statistical error, and further research will be needed to confirm the finding.

"If we were trying to convict Cygnus XR-1 of being a black hole in court, we'd win a civil case that only needs a preponderance of the evidence, but nota criminal case, that requires beyond a reasonable doubt."

, roughly 6,000 light-years away.What he found in images from 1992 were bright flashes of ultraviolet light that sputtered and then disappeared. Dolan suggests that the signals -- he found two separate instances of them -- represent hot blobs of gas orbiting inward and spiraling through the event horizon.
Dolan presented his findings at a meeting of the American Astronomical Society meeting in San Diego, California.
The twilight zone
Cygnus XR-1, with a mass estimated at three to seven times that of our Sun compressed into an area no larger than Earth, is thought to be part of a
. The black hole sucks hot gas off of a large companion star, which is roughly 30 times as massive as our Sun.This gas streams toward the black hole, going into an ever-tighter orbit. Along with other material, the gas forms a flat disk called an accretion disk.
Here's how the gas blobs would disappear, as predicted by the theory of black holes:
As a blob of hot gas approaches the point of no return -- the event horizon -- immense gravity stretches the light waves emanating from the hot gas. At a certain point, the wavelengths are stretched so far that they are no longer visible. The gas then crosses over into a sort of "twilight zone," where time and space no longer obey rules we understand.
Pulse trains
The sequence of pulses Dolan spotted -- six in one event and seven in the other -- each lasted just 0.2 seconds, diminishing in strength with each pulse. And then they were gone. Such an event, if this was one, is called a dying pulse train. (See click-to-enlarge image near the top-right of this page.)
"If pulse trains have clearly been detected, then it is indeed a milestone," said Niel Brandt, assistant professor of astronomy and astrophysics at Penn State. "However, the difficult part is in proving that they have indeed been detected. It is generally difficult to use a complex system, such as an accretion disk around a black hole, as a springboard to address fundamental issues."
The difficulty becomes more pronounced when working with limited data, Brandt told SPACE.com, adding that the finding could spur new research, using similar methods, into Cygnus XR-1 and other black holes in our galaxy.
In an e-mail interview, Dolan emphasized the preliminary nature of the findings.
"If we were trying to convict Cygnus XR-1 of being a black hole in court, we'd win a civil case that only needs a preponderance of the evidence, but not a criminal case, that requires beyond a reasonable doubt," Dolan said. "Finding an even horizon would put the evidence beyond a reasonable doubt."
Dolan notes that observations of many binary star systems suspected of having a black hole have proved that the dense central object is not a white dwarf star or a