A recently discovered black hole
may help astronomers to piece together the family tree of these
enigmatic cosmic objects. While most black holes are classified as
either stellar-mass or the supermassive black holes that can be found at
the center of some galaxies, this new find fits into neither category.
The discovery, called the intermediate-mass black hole (IMBH), has
proved to be a tricky proposition. With a mass somewhere between a few
hundred to a few hundred thousand times that of our own Sun, the size of
these intermediates can vary widely.
This particular black hole was found in an arm of the spiral galaxy
NGC-2276, and has been sensibly named NGC-2276-3c. Lying about 100
million light-years from earth, astronomers were able to tease images
through the use of NASA’s Chandra X-Ray Observatory and the European
Very Long Baseline Interferometry Network.
Although researchers have theorized about the existence of these
IMBHs, locating one has proven elusive until now. A recent
to-be-published paper by an international team of researchers delves
into the specifics of NGC-2276-3c.
“Astronomers have been looking very hard for these medium-sized black
holes,” study co-author Tim Roberts, of the University of Durham in the
United Kingdom, said in a statement. “There have been hints that they
exist, but the IMBHs have been acting like a long-lost relative that
isn’t interested in being found.”
So what was found? It appears that the recently discovery has
characteristics of both the smaller stellar-mass and the much larger
supermassive black holes. It serves as an intermediary between the two,
and some think that these intermediaries are the beginnings of what
could very well become a supermassive.
The team of researchers also noted that the black holes is firing off
super powerful blasts of radio jets. Think of these as material,
traveling at nearly the speed of light and emitting radio waves, which
are thrown out of dense objects. Our newly found black hole is shooting
them out almost 2000 light-years into space. Within a radius of
approximately 1000 light-years around NGC-2276-3c there are no new star
formations, suggesting that the radio jets are pushing out all the gas
necessary for star creation.
The full report on NGC-2276-3c should be appearing shortly in the journal Monthly Notices of the Royal Astronomical Society.
Source Article from http://feedproxy.google.com/~r/AscensionEarth2012/~3/-HVLlmqnCF4/seedling-for-supermassive-black-holes.html
“Seedling” For Supermassive Black Holes Found
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