The image at the bottom of the page was made during the test-phase of the LOFAR telescope, and targeted the giant elliptical galaxy Messier 87 (above), at the center of a galaxy cluster in the constellation of Virgo. This galaxy is 10 times more massive than our Milky Way and hosts in its center one of the most massive black holes discovered so far, with a mass six billion times that of our Sun.
A galaxy and its central black hole lead intimately connected lives, with some black holes actively accrete matter. Part of this material does not fall into the black hole but is ejected in a narrow stream of particles, traveling at nearly the speed of light. When the stream slows down, it creates a tenuous bubble that can engulf the entire galaxy. Invisible to optical telescopes, the bubble is very prominent at low radio frequencies.
Astronomers have produced one of the best images ever of such a bubble, using the LOFARTelescope - designed and built by ASTRON in an international collaboration - ideally suited to detect frequencies from 20 to 160 MHz. "The result is of great importance", says Francesco de Gasperin, lead author of the study that will be published in the journal Astronomy & Astrophysics. "It shows the enormous potential of LOFAR, and provides compelling evidence of the close ties between black hole, host galaxy, and their surroundings."
The LOFAR antenna array is one of the six stations in Germany and 40 stations in the Netherlands that are combined to study the largely unexplored frequency range between 10 and 240 MHz.
M87 is at the center of the Virgo Cluster, a collection of thousands of galaxies that move through space together. It is a giant elliptical galaxy. M87's diameter is only a little bigger than the Milky Way's, but because the galaxy is thicker than the thin disk of the Milky Way, it encompasses a much larger volume. As a result, M87 contains many more stars and is perhaps 10 times as massive as the Milky Way.
Every few minutes this black hole swallows an amount of matter similar to that of Earth, converting part of it into radiation and a larger part into powerful jets of ultra-fast particles, which are responsible for the observed radio emission.
"This is the first time such high-quality images are possible at these low frequencies", says professor Heino Falcke, from Radboud University, Nijmegen, and MPIfR Bonn, chairman of the board of the ILT and co-author of the study. "This was a challenging observation - we did not expect to get such fantastic results so early in the commissioning phase of LOFAR."
To determine the age of the bubble, the authors added radio observations at different frequencies from the Very Large Array in New Mexico (USA), and the Effelsberg 100-meter radio telescope near Bonn (Germany).
The team found that this bubble is surprisingly young, just about 40 million years, which is a mere instant on cosmic time scales. The low frequency observation does not reveal any relic emission outside the well-confined bubble boundaries, this means that the bubble is not just a relic of an activity that happened long ago but is constantly refilled with fresh particles ejected by the central black hole.
"What is particularly fascinating", says Andrea Merloni from the Max-Planck Institute of Extraterrestrial Physics in Garching, who supervised de Gasperin's doctoral work, "is that the results also provide clues on the violent matter-to-energy conversion that occurs very close to the black hole. In this case the black hole is particularly efficient in accelerating the jet, and much less effective in producing visible emission."
Source: The Daily Galaxy via Provided by Max Planck Society