The “Turbulent” Relationship between Stellar Feedback and Magnetic Fields
Turbulence in the magnetic field surrounding a protostar can affect the power and launch angle of bipolar outflows.
A clash of disks: the traumatic life of the HV-DO Tau system
In the right conditions, protoplanetary disks might retain evidence of past encounters and can tell us more about the life story of the stellar environment they reside in.
Connecting galaxy properties to their star-formation histories
Star-forming galaxies form stars at different rates. Could this be the model that reveals the underlying physics?
A Treasure Map of Massive Stars
The authors of today’s paper take us on a treasure hunt of baby massive stars, come join us!
Star Formation Acceleration
Today’s paper discusses a new way to measure physical properties of galaxies—including, for the first time, “star formation acceleration.”
Cradles of Massive Stars
Ever wondered what baby massive stars look like? Let’s find out!