The last breath of the young gigahertz-peaked spectrum radio source PKS 1518+047
M. Orienti, M. Murgia, D. Dallacasa

TL;DR
This study investigates the spectral properties and age of the young, fading gigahertz-peaked spectrum radio source PKS 1518+047 using multi-frequency VLBA and VLA data, revealing its recent shutdown and particle depletion.
Contribution
It provides detailed spectral analysis and age estimation of PKS 1518+047, highlighting its recent cessation of activity and particle depletion, which advances understanding of young radio source evolution.
Findings
Source components have steep spectral indices, indicating no current particle re-acceleration.
Electrons with energies above γ<600 are depleted, with a radiative lifetime of about 2700 years.
The source was active for approximately 2150 years before shutting off, with 20% of its lifetime inactive.
Abstract
We present the results from multi-frequency VLBA observations from 327 MHz to 8.4 GHz of the gigahertz-peaked spectrum radio source PKS 1518+047 (4C 04.51) aimed at studying the spectral index distribution across the source. Further multi-frequency archival VLA data were analysed to constrain the spectral shape of the whole source. The pc-scale resolution provided by the VLBA data allows us to resolve the source structure in several sub-components. The analysis of their synchrotron spectra showed that the source components have steep spectral indices, suggesting that no supply/re-acceleration of fresh particles is currently taking place in any region of the source. By assuming the equipartition magnetic field of 4 mG, we found that only electrons with < 600, are still contributing to the radio spectrum, while electrons with higher energies have been almost completed depleted.…
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