  Emission source functions are extracted from correlation functions
constructed from charged pions produced at mid-rapidity in Au+Au collisions at
sqrt(s_NN)=200 GeV. The source parameters extracted from these functions at low
k_T, give first indications of a long tail for the pion emission source. The
source extension cannot be explained solely by simple kinematic considerations.
The possible role of a halo of secondary pions from resonance emissions is
explored.
