Understanding the surprising narrowness of eccentric debris belts
Some extrasolar debris belts are not just eccentric but also surprisingly narrow. What processes can influence the width of debris belts?
Some extrasolar debris belts are not just eccentric but also surprisingly narrow. What processes can influence the width of debris belts?
Crowned the god of doorway and passages in Roman mythology, Janus had access to the future and the past. In modern times, he is reincarnated into a secret code that turns back time, in computer simulations.
Here’s a long-sought finding for y’all! Read on to find out more.
Orbital stability of high-mass multi-planet systems is scrutinized in comparison to their low-mass counterparts.
Globular clusters are some of the most massive and densest star clusters observed. What are the progenitors of old globular clusters that we see orbiting the Milky Way and other galaxies? What evolutionary and dynamical effects have these clusters experienced? What determines the physical properties of old globular clusters? Why are there two “distinct” classes of globular clusters and what properties determine these physical states? These are the questions the authors aim to answer.