description M1-67 (around WR 124) Overview
M1-67 is an emission nebula surrounding WR 124, a runaway Wolf-Rayet star in the constellation Sagitta. The nebula consists of material expelled by the star and is notable for its irregular, knotty structure, which has been imaged in detail by the Hubble Space Telescope and the James Webb Space Telescope. It is studied as an example of rapid mass loss during the late evolution of a massive star.
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