Radio galaxies are powered by active galactic nuclei, bright central regions associated with matter falling toward supermassive black holes. Some produce jets that feed enormous radio-emitting lobes. When the jets stop, the lobes remain visible for a time as their particles lose energy. Astronomers call these systems remnant radio galaxies.
Researchers led by Sushant Dutta of the University of Cape Town and the Inter-University Institute for Data Intensive Astronomy studied 14 candidate remnants in the XMM-Newton Large-Scale Structure field.
They combined observations from the MeerKAT MIGHTEE and uGMRT superMIGHTEE surveys with data from LOFAR, GMRT and the Karl G. Jansky Very Large Array. Together, the observations covered radio frequencies from 144 MHz to 1.5 GHz.
Models of the sources' radio spectra classified 12 as remnants and reclassified two as active. The result shows why observations at several frequencies are important: candidates selected from limited data can be misidentified.
The models estimated total spectral ages of about 8 million to 42 million years, with a median of roughly 12 million years. These estimates are shorter than those for many remnants examined in earlier studies. The fraction of each source's estimated lifetime spent in the remnant stage ranged from 4% to 83%, suggesting that the sample includes galaxies at very different stages after their jets switched off.
Most of the sources are at relatively high redshifts. The researchers found an association between higher redshift and younger estimated spectral age after accounting for radio luminosity. They said stronger energy losses involving the cosmic microwave background, along with rapid expansion in low-density environments, could help explain the pattern. The observational study does not establish either explanation as the sole cause.
The sample is small, and the ages depend on models of how particles and magnetic fields evolve in the radio lobes. Even so, the findings point to a faint population that previous surveys may have missed. Future surveys with the Square Kilometre Array should find many more such sources and test how common short-lived remnants are.
The study was published in Monthly Notices of the Royal Astronomical Society.
Source: phys.org