Stellar-Wind-Shaped Nebula

Nebula RCW 58

Stars about 100 times more massive than our sun live fast and die young. They burn through their hydrogen supply quickly, then start fusing heavier elements. As they do, their strong stellar winds start blowing off the exterior layers of the star. That’s the story behind WR 40, the star at the center of Nebula RCW 58. The nebula itself is made up of material blown off the star, carved into turbulent filaments by stellar winds. (Image credit: M. Selby and M. Hanson; via APOD)

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