By simulating CO emission with more realistic physics, we find that turbulence measurements from CO lines are typically 10–15% too high, and in some cases up to 40% too high. We provide correction factors to make future measurements more accurate.

This study looks at how well we can measure turbulence in star-forming clouds using CO emission lines. Earlier methods assumed the gas was transparent, but in reality, opacity and radiative transfer affect the signal.

I am also very thankful to the DAAD-WISE fellowship, without which I would not have been able to go to Goettingen!

This work analyses the influence of some parameters on pebble accretion for planets within 1 au of their parent stars. I am incredibly grateful to #MNRAS for accepting my fee waiver and allowing this work to exist outside my VS code.