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Globular star clusters survive 13-billion-year-old massacre

During galaxy collisions, smaller star clusters were destroyed by rapidly changing gravitational forces; only larger clusters survived.
RELATED TOPICS: STARS | STAR CLUSTERS
Two colliding galaxies
Two colliding galaxies based on the new simulation, covering 3.3 billion years. The galaxies eventually merge, destroying many of the stellar clusters (visible here as dots) in the process. Credit: D. Kruijssen, MPA
Our Milky Way Galaxy is surrounded by about 200 compact groups of stars, containing up to a million stars each. At 13 billion years of age, these globular clusters are almost as old as the universe itself and were born when the first generations of stars and galaxies formed.

Now a team of astronomers from Germany and the Netherlands has conducted a novel type of computer simulation that looked at how they were born. They find that these giant clusters of stars are the only survivors of a 13-billion-year-old massacre that destroyed many of their smaller siblings.

Globular clusters have a remarkable characteristic — the typical number of stars they contain appears to be about the same throughout the universe. This is in contrast to much younger star clusters, which can contain almost any number of suns, from fewer than 100 to many thousands. The team of scientists proposes that this difference can be explained by the conditions under which globular clusters formed early in the evolution of their host galaxies.

The researchers ran simulations of isolated and colliding galaxies in which they included a model for the formation and destruction of star clusters. When galaxies collide, they often generate spectacular bursts of star formation (starbursts) and a wealth of bright young star clusters of many different sizes. As a result, it was always thought that the total number of star clusters increases during starbursts. But the Dutch-German team found the opposite result in their simulations.

While the brightest and largest clusters were indeed capable of surviving the galaxy collision due to their own gravitational attraction, the numerous smaller clusters were effectively destroyed by the rapidly changing gravitational forces that typically occur during starbursts due to the movement of gas, dust, and stars. The wave of starbursts came to an end after about 2 billion years, and the researchers were surprised to see that only clusters with high numbers of stars had survived. These clusters had all the characteristics that should be expected for a young population of globular clusters as they would have looked about 11 billion years ago.

“It is ironic to see that starbursts may produce many young stellar clusters, but at the same time also destroy the majority of them,” said Diederik Kruijssen from the Max Planck Institute for Astrophysics in Garching, Germany. “This occurs not only in galaxy collisions, but also should be expected in any starburst environment. In the early universe, starbursts were commonplace; therefore, it makes perfect sense that all globular clusters have approximately the same large number of stars. Their smaller brothers and sisters that didn’t contain as many stars were doomed to be destroyed.”

According to the simulations, most of the star clusters were destroyed shortly after their formation when the galactic environment was still hostile to the young clusters. After this episode ended, the surviving globular clusters have lived quietly until the present day.

The researchers have further suggestions to test their ideas. “In the nearby universe, there are several examples of galaxies that have recently undergone large bursts of star formation,” said Kruijssen. “It should therefore be possible to see the rapid destruction of small stellar clusters in action. If this is, indeed, found by new observations, it will confirm our theory for the origin of globular clusters.”

The simulations suggest that most of a globular cluster’s traits were established when it formed. The fact that globular clusters are comparable everywhere then indicates that the environments in which they formed were very similar, regardless of the galaxy they currently reside in. In that case, Kruijssen believes, they can be used as fossils to shed more light on the conditions in which the first stars and galaxies were born.

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