How Stellar Winds Fuel Sagittarius A*

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How Stellar Winds Fuel Sagittarius A*

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Summary

Astronomers have traced mysterious gas clouds near the center of the Milky Way back to an unexpected origin: the binary star system IRS 16SW. These clouds, part of the so-called G-cloud streamer, follow nearly identical trajectories—strong evidence they share a common source.

Simulations reveal that colliding stellar winds from the binary compress gas into dense clumps, which gradually drift inward toward Sagittarius A*. The result is a direct link between massive stars and black hole feeding, offering new insight into how matter is recycled in one of the most extreme environments in the galaxy.

Thank you for listening to Bedtime Astronomy — your guide to the cosmos. New episodes on space exploration, NASA missions & the latest astronomy breakthroughs.

This episode includes AI-generated content.

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