Rotation and stability of the circumnuclear gas disk in the Galactic Center potential by the ALMA CMZ Exploration Survey (ACES)
Analysis
This article reports on research using the Atacama Large Millimeter/submillimeter Array (ALMA) to study the gas disk around the supermassive black hole at the center of the Milky Way. The focus is on understanding the rotation and stability of this disk, which is crucial for understanding the dynamics of the Galactic Center.
Key Takeaways
Reference
“The article is based on data from the ALMA CMZ Exploration Survey (ACES).”