The development of galactic fountain theories is reviewed with special emph
asis on the different approaches and concepts that have been used in the pa
st. In particular the outstanding contribution of Franz Kahn to our physica
l understanding is appreciated. It is argued that galactic outflows represe
nt an essential phase during galaxy evolution. The dynamics of the outflow
imprints its signature on the emission spectra of soft X-rays, which may we
ll be observable with AXAF and XMM. Finally, some remarks about winds in st
arburst galaxies and AGN are made.