The main outer ring of the WR nebula NGC 2539 expands radially with ve
locity almost-equal-to 26kms-1. The dynamics are modelled as the inter
action of the winds from the 0 progenitor and the present WR stage wit
h clumpy molecular cloud material and Red Supergiant ejecta. In both s
tages, the bubbles are driven by wind momentum. The necessary radiativ
e energy loss probably occurs in boundary layers between cool clumps a
nd hot shocked wind.