[FLASH-USERS] Optically Thin Cooling

[Michiel Bustraan]

Dear all,


I was looking into the radiative capabilities of FLASH.

I've messed around with RadTrans a bit, which takes absorption into account, but also assumes blackbody radiation.


I noticed that the current FLASH userguide refers to a Cooling module which only contains stub level routines (the files themselves don't seem to do anything).

However, in a userguide for FLASH2.5, there is a more detailed description of the optically thin Cooling module.


Is FLASH still capable of modelling optically thin radiative losses?


Kind Regards,

Michiel Bustraan
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