By means of axisymmetric hydrodynamic models with chemistry we study t
he X-ray emission of two processes in a comet : Bremsstrahlung of sola
r wind electrons interacting with the neutral gas coma, and :charge ex
change of heavy solar wind ions in high ionization states with the neu
tral cometary gas. Comparisons of morphology, intensity and spectrum w
ith observations favour heavy ions as the emitting agent (C) 1998 Else
vier Science Ltd. All rights reserved.