VLA image of the M87 radio jet, made at multiple radio frequencies. The jet seen in this image is about 8,000 light-years long. This image clearly shows the corkscrew-like helical structure in the inner part of the jet, which originates at the bright spot at the left, at the core of the galaxy, where a supermassive black hole resides. Credit: Pasetto et al., Sophia Dagnello, NRAO/AUI/NSF. Hi-Res File
VLA image of the M87 radio jet using polarization properties to trace the magnetic field lines in the jet. These lines follow the double-helix structure. Additional analysis shows the direction of the magnetic fields is different at opposite edges of the jet, supporting the conclusion that the magnetic field is helical, like a corkscrew. Credit: Pasetto et al., Sophia Dagnello, NRAO/AUI/NSF. Hi-Res File
Astronomers using the National Science Foundation’s Karl G. Jansky Very Large Array (VLA) have shown that a jet of material propelled from the core of a giant galaxy is channeled by a corkscrew-shaped magnetic field out to nearly 3,300 light-years from the galaxy’s central supermassive black hole. That is much farther than such a magnetic field previously had been detected in a galactic jet.
“By making high-quality VLA images at several different radio wavelengths of the galaxy Messier 87 (M87), we were able to reveal the 3-dimensional structure of the magnetic field in this jet for the first time,” said Alice Pasetto of the National Autonomous University of Mexico, leader of the team. “The material in this jet traces a double helix, similar to the structure of DNA,” she added.
M87 is a giant elliptical galaxy about 55 million light-years from Earth. A supermassive black hole some 6.5 billion times more massive than the Sun lurks at the center of M87. That black hole is the first one ever to be imaged — an achievement done with the world-wide Event Horizon Telescope (EHT) collaboration and announced in 2019. Earlier this year, new EHT images traced the magnetic field in the vicinity of the black hole event horizon.
Pasetto and her colleagues used the VLA to reveal details of the magnetic field by tracing the polarization, or alignment, of radio waves emitted from it, and by measuring the field’s strength across different parts of the jet. Their observations, made using the VLA’s widest configuration that provides the highest resolution, produced very detailed images of the galaxy’s jet.
“Helical magnetic fields are expected close to the black hole, and are thought to play a highly important role in channeling the material into a narrow jet, but we didn’t expect to find such a strong helical field extending so far outward,” said Jose M. Marti, of the University of Valencia.
The magnetic field is expected to weaken with its distance from the black hole. However, the scientists suggested that instabilities in the flow of material within the jet could make the magnetic field more ordered at the distances seen in the new VLA images. The instabilities produce regions of higher pressure which also compress the magnetic field lines.
The astronomers think that this interaction between instabilities in the flow and the magnetic field is what produces the double-helix structure shown by the VLA images. If this is happening in the M87 jet, it likely also is happening in similar jets from galaxies throughout the Universe, they said.
“M87 is relatively near to us and its jet is very powerful, making it an excellent target for study. The clues it gives us can help us understand this very important and ubiquitous phenomenon in the Universe,” said Jose L. Gomez, of IAA-CSIC, Granada.
The scientists are reporting their findings in the Astrophysical Journal Letters.
The National Radio Astronomy Observatory is a facility of the National Science Foundation, operated under cooperative agreement by Associated Universities, Inc.
Media Contact:
Dave Finley, Public Information Officer
(575) 835-7302
dfinley@nrao.edu
Link to Scientific Paper
