Hubble Discovers Groups of Newly Formed Stars in the Tidal Tails of Combining Galactic Systems


Astronomers utilizing the NASA/ESA Hubble Space Telescope have discovered seven interacting galaxy systems featuring extensive, tadpole-like tidal tails composed of gas, dust, and huge numbers of stars. The exceptional clarity and UV light sensitivity of the Hubble Telescope enabled the astronomers to identify 425 clusters of newborn stars within these tidal tails. Each of these clusters can contain up to 1 million freshly formed, blue stars.

The phenomenon of star clusters in tidal tails is not new and has been observed for several decades. It occurs when galaxies interact and gravitational tidal forces draw out long streams of gas and dust. Two well-known examples of this are the Antennae and Mice galaxies, both of which exhibit long, narrow, finger-like projections.

The researchers, led by Michael Rodruck from Randolph-Macon College, combined new observations with existing data to determine the ages and masses of the tidal tail star clusters. The study, published in the Monthly Notices of the Royal Astronomical Society, revealed that these clusters are remarkably young, being only about 10 million years old. Furthermore, it was found that the clusters appear to form at a consistent rate along tails that span thousands of light-years.

These findings challenge previous assumptions and provide new insights into the efficiency of cluster formation. The observations suggest that tidal tails can lead to the creation of new generations of stars that might not have otherwise come into existence.

The process appears to involve the stretching of a galaxy’s spiral arm into space due to the gravitational pull between two interacting galaxies. Prior to their merger, these galaxies contained dense clouds of molecular hydrogen that may have remained inactive. However, during the interaction, these clouds collided and compressed, triggering a surge of star birth.

The future of these elongated star clusters remains uncertain. They may either stay gravitationally intact and evolve into globular star clusters, similar to those that orbit outside our Milky Way Galaxy, or disperse to form a halo of stars around their host galaxy. Alternatively, they may be ejected into intergalactic space. This “string-of-pearls” star formation process may have been more prevalent in the early universe when galaxy collisions were more frequent. The galaxies observed by Hubble serve as significant proxies for understanding past cosmic events.



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