Cloud Collisions Ignite Star Clusters ✎ express

Original: "Cloud-Cloud Collisions Induce Filament-Mediated Super Star Cluster Formation in the Antennae Overlap Region: Evidence from ALMA and JWST"
arXiv:2602.01616 · 2026-02-02 · arXiv non-exclusive · independent analysis · 1 min
In the colliding Antennae Galaxies, giant gas clouds smash into each other and give birth to super star clusters.

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In the Antennae Galaxies, which are crashing into each other, giant gas clouds collided at a speed of 50 kilometers per second. It's like two trains hurtling toward each other — the impact compressed the gas, and it ignited with new stars.

Scientists aimed the ALMA radio telescope at the collision site and saw two clouds that were once a single entity. One cloud stretched into a long filament, curved like a ribbon in the wind, while the other gathered into a knot with fibers extending from it. At the junction of these structures, radio waves revealed hot gas ionized by the radiation of young stars. Nearby, the JWST infrared telescope spotted the glow of dust warmed by newborn luminaries.

Super star clusters are spherical groups of tens of thousands of stars born at once. Our Galaxy has almost none, but in colliding galaxies they are common.

Such clusters are rare guests in quiet galaxies, but in merger zones they appear one after another. Now it's clear why: cloud collisions compress gas so strongly that it transforms all at once into a dense swarm of stars. It's as if two swarms of bees flew into each other and merged into one giant hive.

The collision speed of the clouds—50 km/s — is 100 times faster than the fastest aircraft. At such an impact, the gas compresses hundreds of times, and it is this compression that triggers the birth of thousands of stars.

In Isaac Asimov's novel 'The Gods Themselves,' the collision of two universes generates energy. Here, on a smaller scale, the collision of two clouds generates the light of thousands of new stars.

Scientists
Ludwig BoltzmannFritz ZwickySubrahmanyan ChandrasekharEnrico FermiRashid Alievich SunyaevJames Jeans
Concepts
star formation regions star formation in clusters clump open cluster galaxy cluster shadow dense clump molecular cloud intracluster medium galaxy merger signatures starburst dark interstellar cloud galactic halo composition galactic outflow acceleration solar storm interstellar dust constellation Sunyaev–Zeldovich effect stellar flares stellar chemical abundances bubble collision