Investigating the Origin of the Gas in the Debris Disk Around 49 Ceti
Live Poster Session: Zoom Link Abstract: Circumstellar disks are flat structures of gas and dust around main sequence stars, analogous to the Kuiper belt in our own solar system. Younger disks tend to be gas-rich, while older disks, called debris disks, tend to be gas-poor. However, gas has been detected in an increasing number of … Read more