Maximum Brightness Temperature of an Incoherent Synchrotron Source : Inverse Compton Limit - a Misnomer

We show that an upper limit of ∼ 10 K on the peak brightness temperature for an incoherent synchrotron radio source, commonly referred to in the literature as an inverse Compton limit, may not really be due to inverse Compton effects. We show that a somewhat tighter limit Teq ∼ 10 11 is actually obtained for the condition of equipartition of energy between radiating particles and magnetic fields which happens to be a configuration of minimum energy for a selfabsorbed synchrotron radio source. An order of magnitude change in brightness temperature from Teq in either direction would require departures from equipartition of about eight orders of magnitude, implying a change in total energy of the system up to ∼ 10 times the equipartition value. Constraints of such extreme energy variations imply that brightness temperatures may not depart much from Teq. This is supported by the fact that at the spectral turnover, brightness temperatures much lower than∼ 10 K are also not seen in VLBI observations. Higher brightness temperatures in particular, would require in the source not only many orders of magnitude higher additional energy for the relativistic particles but also many order of magnitude weaker magnetic fields. Diamagnetic effects do not allow such extreme conditions, keeping the brightness temperatures close to the equipartition value, which is well below the limit where inverse Compton effects become important. Subject headings: galaxies: active — quasars: general — radiation mechanisms: non-thermal — radio continuum: general