Astronomers have used two Australian radio telescopes and several optical telescopes to study complex mechanisms that are fuelling jets of material blasting away from a black hole 55 million times more massive than the Sun.
The giant radio galaxy Centaurus A as observed by the Murchison Widefield Array telescope [Credit: Credit ICRAR/Curtin] |
"As the closest radio galaxy to Earth, Centaurus A is the perfect 'cosmic laboratory' to study the physical processes responsible for moving material and energy away from the galaxy's core," said Dr Ben McKinley from the International Centre for Radio Astronomy Research (ICRAR) and Curtin University in Perth, Western Australia.
Centaurus A is 12 million light-years away from Earth—just down the road in astronomical terms—and is a popular target for amateur and professional astronomers in the Southern Hemisphere due to its size, elegant dust lanes, and prominent plumes of material.
Centaurus A observed at 154 MHz by the Murchison Widefield Array [Credit: ICRAR/Curtin] |
"We used the Murchison Widefield Array (MWA) and Parkes—these radio telescopes both have large fields of view, allowing them to image a large portion of sky and see all of Centaurus A at once. The MWA also has superb sensitivity allowing the large-scale structure of Centaurus A to be imaged in great detail," he said.
The MWA is a low frequency radio telescope located at the Murchison Radio-astronomy Observatory in Western Australia's Mid West, operated by Curtin University on behalf of an international consortium. The Parkes Observatory is 64-metre radio telescope commonly known as "the Dish" located in New South Wales and operated by CSIRO.
A close-up view of Centaurus A and the location of a black hole 55 million times more massive than the Sun [Credit: ICRAR/Curtin] |
"If we can figure out what's going in Centaurus A, we can apply this knowledge to our theories and simulations for how galaxies evolve throughout the entire Universe," said co-author Professor Steven Tingay from Curtin University and ICRAR.
"As well as the plasma that's fuelling the large plumes of material the galaxy is famous for, we found evidence of a galactic wind that's never been seen—this is basically a high speed stream of particles moving away from the galaxy's core, taking energy and material with it as it impacts the surrounding environment," he said.
Source: The International Centre for Radio Astronomy Research [December 12, 2017]