Radiation from massive stars can melt away protoplanetary disks. What can the leftover disks tell us about the environment from which they formed?
Star-forming galaxies form stars at different rates. Could this be the model that reveals the underlying physics?
The authors of today’s paper take us on a treasure hunt of baby massive stars, come join us!
Today’s paper discusses a new way to measure physical properties of galaxies—including, for the first time, “star formation acceleration.”
Ever wondered what baby massive stars look like? Let’s find out!
Star clusters may form in a similar way to the hierarchical formation of galaxies, let’s find out how it works!