Closed will-henney closed 12 years ago
We can use the Esteban (2004) abundances for the nebula. Of course, we have to make a decision whether to use the t^2=0 or t^2=0.002 version, and whether to use the ORL or CEL values...
These new abundance sets are now added in emission branch
The easiest way to o this would just be to scale the emissivities by the correction to the abundance.
However, there may be secondary effects due to changes in the thermal structure, although these are unlikely to be important if it is just a few elements such as Fe that are changing.