Telescope detects unprecedented behaviour from nearby magnetar

Publicly released:
Australia; NSW; VIC
Carl Knox, OzGrav/Swinburne University of Technology
Carl Knox, OzGrav/Swinburne University of Technology

Captured by cutting-edge radio telescope technology, a chance reactivation of a magnetar – the Universe’s most powerful magnets – has revealed an unexpectedly complex environment.

Media release

From: CSIRO

Researchers using Murriyang, CSIRO’s Parkes radio telescope, have detected unusual radio pulses from a previously dormant star with a powerful magnetic field.

New results published today in Nature Astronomy describe radio signals from magnetar XTE J1810-197 behaving in complex ways.

Magnetars are a type of neutron star and the strongest magnets in the Universe. At roughly 8,000 light years away, this magnetar is also the closest known to Earth.

Most are known to emit polarised light, though the light this magnetar is emitting is circularly polarised, where the light appears to spiral as it moves through space.

Dr Marcus Lower, a postdoctoral fellow at Australia’s national science agency – CSIRO, led the latest research and said the results are unexpected and totally unprecedented.

"Unlike the radio signals we've seen from other magnetars, this one is emitting enormous amounts of rapidly changing circular polarisation. We had never seen anything like this before,” Dr Lower said.

Dr Manisha Caleb from the University of Sydney and co-author on the study said studying magnetars offers insights into the physics of intense magnetic fields and the environments these create.

"The signals emitted from this magnetar imply that interactions at the surface of the star are more complex than previous theoretical explanations.”

Detecting radio pulses from magnetars is already extremely rare: XTE J1810-197 is one of only a handful known to produce them.

While it’s not certain why this magnetar is behaving so differently, the team has an idea.

“Our results suggest there is a superheated plasma above the magnetar's magnetic pole, which is acting like a polarising filter,” Dr Lower said.

“How exactly the plasma is doing this is still to be determined.”

XTE J1810-197 was first observed to emit radio signals in 2003. Then it went silent for well over a decade. The signals were again detected by the University of Manchester's 76-m Lovell telescope at the Jodrell Bank Observatory in 2018 and quickly followed up by Murriyang, which has been crucial to observing the magnetar’s radio emissions ever since.

The 64-m diameter telescope on Wiradjuri Country is equipped with a cutting edge ultra-wide bandwidth receiver. The receiver was designed by CSIRO engineers who are world leaders in developing technologies for radio astronomy applications.

The receiver allows for more precise measurements of celestial objects, especially magnetars, as it is highly sensitive to changes in brightness and polarisation across a broad range of radio frequencies.

Studies of magnetars such as these provide insights into a range of extreme and unusual phenomena, such as plasma dynamics, bursts of X-rays and gamma-rays, and potentially fast radio bursts.

CSIRO acknowledges the Wiradjuri People as the traditional custodians of the Parkes Observatory site where Murriyang, our Parkes radio telescope, is located.

Multimedia

Murriyang, CSIRO's Parkes radio telescope
Murriyang, CSIRO's Parkes radio telescope
magnetar_medusa.wav
magnetar_medusa.wav

Attachments

Note: Not all attachments are visible to the general public. Research URLs will go live after the embargo ends.

Other CSIRO, Web page Media assets
Journal/
conference:
Nature Astronomy
Research:Paper
Organisation/s: CSIRO, The University of Sydney, Swinburne University of Technology, Western Sydney University
Funder: Murriyang, CSIRO's Parkes radio telescope is part of the Australia Telescope National Facility (https: //ror.org/05qajvd42) which is funded by the Australian Government for operation as a National Facility managed by CSIRO. Pulsar research at the Jodrell Bank Centre for Astrophysics and Jodrell Bank Observatory is supported by a consolidated grant from the UK Science and Technology Facilities Council (STFC). This paper includes archived data obtained through the CSIRO Data Access Portal (http://data.csiro.au). Data reduction, analysis and computations were performed on the OzSTAR national HPC facility, which is funded by Swinburne University of Technology and the National Collaborative Research Infrastructure Strategy (NCRIS). This research was funded partially by the Australian Government through the Australian Research Council (ARC) grant CE170100004 (OzGrav). R.M.S. acknowledges support through ARC Discovery Project DP220102305 and ARC Future Fellowship FT190100155. M.C. acknowledges support of an ARC Discovery Early Career Research Award DE220100819 funded by the Australian Government and the ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO3D),through project number CE170100013. S.D. is the recipient of an ARC Discovery Early Career Award (DE210101738) funded by the Australian Government. D.L. acknowledges the National Natural Science Foundation of China #11988101. K.M.R. acknowledges support from the Vici research programme “ARGO” with project number 639.043.815, financed by the Dutch Research Council (NWO).
Media Contact/s
Contact details are only visible to registered journalists.