Cosmic Necklace Reveals Secrets of Galaxy Birth ✛

Original: "Bright [CII]158$$\mu$$m Streamers as a Beacon for Giant Galaxy Formation in SPT2349$$-$$56 at $$z=4.3$$"
arXiv:2509.08035 · 2025-09-09 · CC BY 4.0 · 1 min
Three colliding galaxies ejected gas that curled into glowing beads on an invisible thread — this is how a cosmic giant is born.

Three giant galaxies collide, and from the impact, gas flies away. But it does not disappear without a trace — it compresses into clumps resembling beads of a cosmic necklace, strung on an invisible thread spanning thousands of light-years. The light from these beads comes from atoms of carbon heated by shock waves — like the air in front of a supersonic jet, only on a galactic scale.

It's amazing that the gas remains colder than ice on Earth (minus 243°C), but glows due to intense heating from the collision. In this necklace, stars are born at a furious rate: thousands of new suns appear each year, while our Milky Way creates just a couple. Spectroscopy — breaking light into colors — allows us to peer into these processes, and observations are conducted at wavelengths where cold cosmic dust and gas shine.

Such a cataclysm is not chaos, but construction: from these beads, giant elliptical galaxies later form, the most massive in the Universe.

The gas 'beads' are heated only to -243°C — 20 degrees colder than Pluto's surface. But thanks to shock waves, they glow so brightly that they can be detected at a distance of billions of light-years.

Scientists
Ludwig BoltzmannFritz ZwickyRashid Alievich SunyaevRainer SachsJames JeansCecilia Payne-Gaposchkin
Concepts
starburst population iii stars first stars m87 star formation in clusters open cluster stellar stream hot gas spiral galaxy red giant galaxy formation galactic center progenitor dense clump outburst intracluster medium galactic bulge globular cluster stellar nursery gamma ray burst merger