A new associated pumping mechanism for masers in regions of star formation
is presented, giving a unified interpretation for both H2O and OH interstel
lar masers. A very wide range of photons contributes to this mechanism, thu
s sufficient numbers of photons are available. A reasonable mechanism for t
he regeneration of interstellar H2O and OH molecules is presented. Therefor
e this model overcomes several drawbacks of former radiative mechanisms. It
is both simple and compatible with astronomical conditions.