Hubble Finds Clusters of Newborn Stars in Tidal Tails of Merging Galaxy Systems

Using the NASA/ESA Hubble Space Telescope, astronomers have observed seven interacting galaxy systems that have long, tadpole-like tidal tails of gas, dust, and a plethora of stars. Hubble’s exquisite sharpness and sensitivity to ultraviolet light have uncovered 425 clusters of newborn stars along these tidal tails; each cluster contains as many as 1 million blue, newborn stars.

Star clusters in tidal tails have been known about for decades. When galaxies interact, gravitational tidal forces pull out long streamers of gas and dust.

Two popular examples are the Antennae and Mice galaxies with their long, narrow, finger-like projections.

In the new research, Randolph-Macon College astronomer Michael Rodruck and colleagues used a combination of new observations and archival data to get ages and masses of tidal tail star clusters.

The researchers found that these clusters are very young — only 10 million years old.

And they seem to be forming at the same rate along tails stretching for thousands of light-years.

“It’s a surprise to see lots of the young objects in the tails,” said Dr. Rodruck, lead author of a paper published in the Monthly Notices of the Royal Astronomical Society.

“It tells us a lot about cluster formation efficiency.”

“With tidal tails, you will build up new generations of stars that otherwise might not have existed.”

The tidal tails look like they are taking a galaxy’s spiral arm and stretching it out into space.

The exterior part of the arm gets pulled like taffy from the gravitational tug-of-war between a pair of interacting galaxies.

Before the mergers, the galaxies were rich in dusty clouds of molecular hydrogen that simply may have remained inert.

But the clouds got jostled and bumped into each other during the encounters.

This compressed the hydrogen to the point where it precipitated a firestorm of star birth.

“The fate of these strung-out star clusters is uncertain,” the astronomers said.

“They may stay gravitationally intact and evolve into globular star clusters — like those that orbit outside the plane of our Milky Way Galaxy.”

“Or they may disperse to form a halo of stars around their host galaxy, or get cast off to become wandering intergalactic stars.”

“This string-of-pearls star formation may have been more common in the early Universe when galaxies collided with each other more frequently.”

“These nearby galaxies observed by Hubble are a proxy for what happened long ago, and therefore are laboratories for looking into the distant past.”

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Michael Rodruck et al. 2023. Star clusters in tidal debris. MNRAS 526 (2): 2341-2364; doi: 10.1093/mnras/stad2886