› Forums › Comets › distribution of C2 › Not CN rate of dissociation
31 January 2022 at 2:12 pm
#585190
![](https://britastro.org/wp-content/uploads/2016/11/picture-146-1478110706-80x80.jpg)
Participant
“Is CN also broken down by sunlight, though at perhaps a slower rate than C2 ?”
Actually, answering my own question it looks like that cannot be the explanation as CN is seen widely distributed in the cross section through the tail of 2020 F3. Any ideas of what is going on?