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Pinpointing origin of gamma rays from a supermassive black hole
The chart below describes results of the study "Radio Imaging of the Very-High-Energy Gamma-Ray Emission Region in the Central Engine of a Radio Galaxy," which appears in the July 2 Science Express. The upper panel shows the very-high-energy gamma-ray emission from the radio galaxy M87 during 2007-2008 measured with the VERITAS, H.E.S.S and MAGIC experiments. The regular gaps in the light curve correspond to phases of full moon during which no observations were possible. The vertical gray box indicates the time period of the strong flaring activity. The lower panel shows the radio flux as measured with the Very Long Baseline Array, which detects radio waves with high spatial precision, from a region very close to the supermassive black hole in M87. Credit: The VERITAS Collaboration, the VLBA 43 GHz M 87 Monitoring Team, the H.E.S.S. Collaboration, and the MAGIC Collaboration.
An international collaboration of 390 scientists reports the discovery of an outburst of very-high-energy (VHE) gamma radiation from the giant radio galaxy Messier 87 (M 87), accompanied by a strong rise of the radio flux measured from the direct vicinity of its super-massive black hole.
The combined results give first experimental evidence that particles are accelerated to extremely high energies of tera electron Volt (one electron Volt is the energy an electron or proton gains when it is accelerated by a voltage of one Volt) in the immediate vicinity of a supermassive black hole and then emit the observed gamma rays. The gamma rays have energies a trillion times higher than the energy of visible light.
The large collaborative effort involved three arrays of 12-meter to 17-meter telescopes that detect very high-energy gamma rays and the Very Long Baseline Array (VLBA) that detects radio waves with high spatial precision.
Washington University in St. Louis scientists Matthias Beilicke, Ph.D., postdoctoral research associate in physics in Arts & Sciences, and Henric Krawczynski, Ph.D., associate professor of physics, working with VERITAS (Very Energetic Radiation Imaging Telescope Array System), coordinated this cooperative project for the VERITAS collaboration, the results of which will appear in the July 2 Science Express, the advance online publication of the journal Science.
"We had scheduled gamma-ray observations
"Only combining the high-resolution radio observations with the VHE gamma-ray observations allowed us to locate the site of the gamma-ray production," says R. Craig Walker, Ph.D., staff scientist at the National Radio Astronomy Observatory in Socorro, New Mexico.
M 87 is located at a distance of 50 million light years from Earth in the Virgo cluster of galaxies. The black hole in the center of M 87 is six billion times more massive than the Sun. The size of a non-rotating black hole is given by the Schwarzschild radius. Everything — matter or radiation — that comes within one Schwarzschild radius of the center of the black hole will be swallowed by it. The Schwarzschild radius of the supermassive black hole in M 87 is comparable to the radius of our Solar System.
In the case of some supermassive black holes — as in M 87 — matter orbiting and approaching the black hole powers highly relativistic outflows, called jets. The matter in the jets travels away from the black hole, escaping its deadly gravitational force. The jets are some of the largest objects in the Universe, and they can reach out many thousands of light years from the vicinity of the black hole into the intergalactic medium.
VHE gamma-ray emission from M 87 was first discovered in 1998 with the HEGRA Cherenkov telescopes. "But even today, M 87 is one of only about 25 sources outside our galaxy known to emit VHE gamma rays," says Beilicke.
The new observations now show that the particle acceleration, and the subsequent emission of gamma rays, can happen in the very "inner jet," less than about 100
In addition to VERITAS and the VLBA, the High Energy Stereoscopic System (H.E.S.S.) and the Major Atmospheric Gamma-Ray Imaging
Measurement of VHE gamma rays with Cherenkov telescopes
The VHE gamma rays with energies ranging from hundred GeV (one billion electron Volt)
The Cherenkov telescopes detect the faint, extremely short flashes of blue light, which these particles emit (named Cherenkov light) using extremely sensitive cameras. The images can be used to infer the arrival direction and initial energy of the primary gamma rays.
The three telescope systems involved in the observations are located in Arizona, USA (VERITAS); Namibia, Africa (H.E.S.S.); and on the Canary Island La Palma, Spain (MAGIC).
Coordinating the observations between the three experiments resulted in an observation of time of about 120 hours in 2008, allowing for the detection of the strong gamma-ray flares.
High-resolution radio imaging with VLBA
The VLBA is a system of 10 radio-telescope antennas, each with a dish 25 meters (82 feet) in diameter and weighing 240 tons. From Mauna Kea on the Big Island of Hawaii to St. Croix in the U.S. Virgin Islands, the VLBA spans more than 5,000 miles, providing astronomers with the sharpest vision of any telescope on Earth or in space.
Dedicated in 1993, the VLBA has an ability to see fine detail equivalent to being able to stand in New York and read a newspaper in Los Angeles. From January 2007 to April 2008, Craig Walker and co-workers used the VLBA
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Washington University in St. Louis: http://www.wustl.edu Thanks to Washington University in St. Louis for this article.
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