Hi Ken,
A very nice capture of this object, but I would propose a different approach to get the 'true' colors of Ha-OIII emission nebulae, based on their physical properties.
Hydrogen has two strong emission lines in the visible spectrum, Ha(red) and Hb(blue).
OIII(green/blue) is located at the transition of green to blue.
I therefore map the channels like this:
R = Ha
G = OIII
B = OIII+0.15*Ha
This gives a very natural color rendition of emission nebulae.
Best regards,
Gerhard