  Using a (3+1)-dimensional solution of the relativistic Euler-equations for
$Pb+Pb$ at 160 $AGeV$, space-time extensions of kaon emission zones are
calculated from space-time densities and compared to the inverse widths of
two-kaon Bose-Einstein correlation functions. The comparison shows a
satisfactory agreement and it is concluded that because of the Gaussian shape
of the kaon correlation functions, the space-time parameters of the kaon source
can be calculated directly from space-time densities. In the case of intensity
interferometry of identical pions this simplification is not recommended when
applying Gaussian fits because of the present strong effects of resonance
decays. The whole discussion is based on the assumption that hadron emission in
ultra-relativistic heavy-ion collisions is purely chaotic or that coherence is
at least negligible.
