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Lone, starless cloud may be a 'dark' galaxy

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Astronomers using China's FAST radio telescope have discovered a compact hydrogen cloud devoid of visible stars. Containing nearly 500,000 solar masses of neutral hydrogen, it represents one of the strongest candidates yet for an isolated dark galaxy.

Unusual Detection by the FAST Telescope

Astronomers exploring the hidden structures of the cosmos have uncovered an intriguing candidate. Utilizing China's massive FAST radio telescope, researchers detected a compact gas cloud isolated from any visible stars or neighboring galactic systems. The discovery paper detailing the observation was posted to the arXiv preprint server on September 24.

Physical Properties of the Starless Cloud

Measurements gathered at radio wavelengths revealed that this mysterious cloud contains nearly 500,000 times the sun's mass in neutral hydrogen. While substantial reservoirs of neutral hydrogen typically trigger star formation, optical observations show no accompanying starlight whatsoever. This compact, isolated configuration suggests a reservoir of primordial gas that has remained completely devoid of star-forming activity.

Significance for Dark Galaxy Hypotheses

The discovery stands as one of the strongest candidates yet for an isolated 'dark galaxy.' Probing starless gas clouds that hold significant hydrogen mass provides critical observational data for testing galaxy formation frameworks and deepening our understanding of how dark matter halos gather and retain baryonic gas.

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