Young Stars: Gamma Rays from Jets express

Original: "Evidence for protostellar jets as a population of hadronic gamma-ray sources"
arXiv:2606.19445 · 2026-06-17 · CC BY 4.0 · 1 min
Newborn stars have been found emitting gamma rays: their jets accelerate protons, which produce powerful radiation.

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Stars are born in cold clouds of cosmic dust and hydrogen. Inside these cocoons, protostars — the cores of future suns — were long thought to be just hot clumps. But it turns out many of them are powerful accelerators: they shoot out narrow jets of gas that, slamming into surrounding matter, produce invisible gamma-ray light.

The situation is like a high-pressure hose blasting water at a wall: the spray fans out. Here, the jet is a stream of protons accelerated to nearly the speed of light, and the spray is gamma rays. This "glow" can punch through even thick dust, letting telescopes peer into opaque stellar nurseries.

These protostars are scattered throughout the Milky Way. The brighter the star in ordinary light (its total luminosity), the more powerful its gamma-ray jets. This means that particle acceleration is a key stage in a star's coming of age. Gamma rays help us study how stars churn up material in their cradles, influencing the birth of planets.

Protostellar jets accelerate protons to 99.99% the speed of light — faster than any human-made particle accelerator.

Scientists
Bernhard RiemannJoseph WeberKarl SchwarzschildKip ThorneRainer WeissAlbert Einstein
Concepts
star formation gas young star first stars stellar nursery protoplanetary disk population iii stars young stellar object protoplanetary disk chemistry galaxy formation starburst gas supernova jets galactic dust winds galaxy growth mechanisms gap dust dynamics galactic evolution processes cosmic dawn molecular cloud open cluster