Abstract
We report on ROSAT HRI observations of the nearby powerful radio galaxies 3C33 and 3C111, which both have detected optical hot spots. We find nuclear X-ray sources in both objects, but no X-ray emission from the hot spots. This confirms the presence of a high-energy cutoff in the spectrum of synchrotron-emitting electrons. Since these electrons necessarily scatter the synchrotron photons by the inverse-Compton process, our upper limits on the X-ray fluxes of the hot spots allow us to set lower limits of a few nanotesla on their magnetic flux density, close to or greater than the fields implied by equipartition of energy between radiating particles and magnetic field.
| Original language | English |
|---|---|
| Pages (from-to) | 615-621 |
| Journal | Monthly Notices of the Royal Astronomical Society (MNRAS) |
| Volume | 294 |
| Issue number | 4 |
| DOIs | |
| Publication status | Published - 1998 |
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