Astronomers using the Hubble Space Telescope (HST) have studied one of the largest young star clusters in our galaxy, Westerlund 1.
The cluster is not perfectly round, but stretched out in a northeast-southwest direction, with an eccentricity of 0.71.
Westerlund 1 has a velocity dispersion lower than expected, suggesting it formed with high efficiency or experienced minimal disruption after its birth.
The study provides important insights into the evolution and formation history of massive young star clusters, supporting the idea of mass segregation.