Astronomers using the National Science Foundation’s Karl G. Jansky Very Large Array (VLA) have discovered new details that are helping them decipher the mystery of how giant radio-emitting structures are formed at the center of a cluster of galaxies.
The scientists studied a cluster of thousands of galaxies more than
250 million light-years from Earth, named the Perseus Cluster after the
constellation in which it appears. Embedded within the center, the
Perseus Cluster hosts a pool of superfast particles that emit radio
waves, creating a radio structure known as a “mini-halo.” Mini-haloes
have been found in about 30 galaxy clusters, but the halo in the Perseus
Cluster is the largest known, about 1.3 million light-years in
diameter, or 10 times the size of our Milky Way Galaxy.
The sizes of the mini-haloes have presented a puzzle to astronomers.
As the particles travel away from the cluster’s center, they should slow
down and stop emitting radio waves long before they reach the distances
observed, according to theory.
“At large distances from the central galaxy, we don’t expect to be
able to see these haloes,” said Marie-Lou Gendron-Marsolais, of the
University of Montreal. “However, we do see them and we want to know
why,” she added.
The astronomers took advantage of the upgraded capabilities of the
VLA to make new images of the Perseus Cluster that were both more
sensitive to fainter radio emissions and provided higher resolution than
previous radio observations.
“The new VLA images provided an unprecedented view of the mini-halo
by revealing a multitude of new structures within it,” said Julie
Hlavacek-Larrondo, also of the University of Montreal. “These structures
tell us that the origin of the radio emission is not as simple as we
thought,” she said.
The new details indicate that the halo’s radio emission is caused by
complex mechanisms that vary throughout the cluster. As theorized
before, some radio emission is caused by particles being reaccelerated
when small groups of galaxies collide with the cluster and give the
particles a gravitational shove. In addition, however, the scientists
now think that the radio emission is also caused by the powerful jets of
particles generated by the supermassive black hole at the core of the
central galaxy that give an extra “kick” of energy to the particles.
“This would help explain the rich variety of complex structures that we see,” Gendron-Marsolais said.
“The high-quality images that the upgraded VLA can produce will be
key to helping us gain new insights into these mini-haloes in our quest
to understand their origin,” Hlavacek-Larrondo said. The VLA, built
during the 1970s, was equipped with all-new electronics to bring it up
to the technological state of the art by a decade-long project completed
in 2012.
Gendron-Marsolais and Hlavacek-Larrondo, along with an international team of researchers, are reporting their findings in the Monthly Notices of the Royal Astronomical Society.
The National Radio Astronomy Observatory is a facility of the
National Science Foundation, operated under cooperative agreement by
Associated Universities, Inc.
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