If you have an atom, e.g., prepared to be at rest in your (inertial) reference frame, this means that its center of mass is not moving but that the nucleus and the electron are moving around each other (taken the average positions of these "particles" as their position). You don't need esoterics for this but just quantum theory in the minimal interpretation.
Now to see, what's about radiation emitted from the atom you have to work in full QED, i.e., you have to consider the system of the nucleus, the electrons, and the quantized radiation field. Provided the atom is isolated from its environment (FAPP), then it does not radiate if and only if its in the ground state. All other bound states of the perturbative treatment, where the interaction with the em. radiation field is neglected are in fact instable when the coupling to the radiation field is taken into account. The atom will rearrange itself in the ground state emitting one or more photons in this process. The photons have a small but finite width, which is inverse to the mean lifetime of the excited states.
Of course, it's not to be confused with classical bremsstrahlung from the charged particles within the atom. This phenomenon of the stability of atoms (in the strict sense in the ground state) cannot be understood in classical terms and this was one of the facts that lead to the discovery of quantum theory in 1925/26.
Bohrs model of 1911/12 and Sommerfeld's extension was an important step towards this discovery, but it's in almost all aspects wrong, even qualitatively. There are no "Bohr orbits", and consequently there's no necessity ad-hoc assumption about "orbits, where the electron doesn't rotate". The only way to understand the atom is quantum theory. You can go quite far with non-relativistic quantum theory in the semiclassical limit (i.e., treating the em. field as a classical Coulomb potential rather than the full QED treatment, and this can be proven from QED; see, e.g., the excellent QED treatment of the hydrogen atom in Weinberg's Quantum Theory of Fields, vol. 1).