SIMBAD references

We investigate the X-ray properties of the powerful radio galaxy Hercules A (3C 348) using ROSAT HRI, PSPC and ASCA observations. The ASCA data are well fit by a thermal plasma model with a temperature of about 4.3keV and abundances 0.4 solar. The HRI observation clearly reveals extended and elongated X-ray emission. For radii greater than 10 arcsec, the surface brightness profile perpendicular to the elongation is well fit by an isothermal β-model with β= 0.63 and a core radius of ≃120 kpc. We derive a total mass of the putative cluster of 8.4x10¹³ M_☉ and a gas mass fraction of about 18 per cent. The inner part of the surface brightness profile clealry reveals the presence of a point source, which contributes ≃8 per cent to the total flux. The 0.1-2.4keV luminosity of the point-like and the extended emission is 3.4x10⁴³ and 4.3x10⁴⁴erg/s, respectively. After subtracting the cluster X-ray emission from the HRI image, residual structures are visible, which partly coincide with the radio jet and lobes. This indicates an interaction of the radio jet with the intracluster medium.