When planets form, where should they move? Towards their host star? In the other direction? The authors of today’s paper show that this is not obvious!
Some things are really hard to observe, but we still can study them using computer simulations! Today’s paper will show you how people study planets-driven spiral arms!
Forbidden emission lines can trace photoevaporative winds in protoplanetary disks. What will those lines reveal? Find out in today’s guest post!
It’s nice to have the conclusion of a paper in its title – Super-Jupiters migrate outward. Today, let’s investigate what exactly this means!
The closest look yet at the mysterious outflows from high mass newborn stars.
In this guest post, Tony Rodríguez describes how the environments of planet formation may not be so simple (and sticky!) after all.