Suzaku diagnostics of the energetics in the lobes of the giant radio galaxy 3C 35
Naoki Isobe, Hiromi Seta, Poshak Gandhi, Makoto S. Tashiro

TL;DR
This study used Suzaku X-ray observations to analyze the energetics of the radio lobes in galaxy 3C 35, revealing low energy densities and near equipartition between particles and magnetic fields.
Contribution
First detailed Suzaku X-ray analysis of 3C 35's lobes, quantifying electron and magnetic energy densities and confirming near equipartition.
Findings
X-ray emission from lobes attributed to inverse Compton scattering.
Electron energy density is the lowest among studied radio galaxy lobes.
Magnetic field strength estimated at approximately 0.88 microGauss.
Abstract
The Suzaku observation of a giant radio galaxy 3C 35 revealed faint extended X-ray emission, associated with its radio lobes and/or host galaxy. After careful subtraction of the X-ray and non-X-ray background and contaminating X-ray sources, the X-ray spectrum of the faint emission was reproduced by a sum of the power-law (PL) and soft thermal components. The soft component was attributed to the thermal plasma emission from the host galaxy. The photon index of the PL component, where the first and second errors represent the statistical and systematic ones, was found to agree with the synchrotron radio index from the lobes, . Thus, the PL component was attributed to the inverse Compton (IC) X-rays from the synchrotron electrons in the lobes. The X-ray flux density at 1 keV was derived as …
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