A two-year cycle in the gamma-ray brightness of a blazar, a galaxy powered by a supermassive black hole, has been confirmed by 10 years of observations from NASA's Fermi Gamma-ray Space Telescope. The findings were announced today at the Eighth International Fermi Symposium meeting this week in Baltimore.
"This is the first time that a gamma-ray period has been confirmed in an active galaxy," said Stefano Ciprini, a researcher at the INFN Tor Vergata division of the Italian Space Agency's Space Science Data Center in Rome. "The gamma-ray period is also seen in other wavebands, including visible light, and additional X-ray and radio data hint at similar brightness peaks."
Some of the matter falling into the blazar, named PG 1553+113, forms a jet of particles that radiates gamma rays, the highest-energy form of light, almost directly toward Earth.
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"This is the first time that a gamma-ray period has been confirmed in an active galaxy," said Stefano Ciprini, a researcher at the INFN Tor Vergata division of the Italian Space Agency's Space Science Data Center in Rome. "The gamma-ray period is also seen in other wavebands, including visible light, and additional X-ray and radio data hint at similar brightness peaks."
Some of the matter falling into the blazar, named PG 1553+113, forms a jet of particles that radiates gamma rays, the highest-energy form of light, almost directly toward Earth.
Continued...
Source