Linked from

The 68 pages that link to Stellar wind, each with the reason it gives.

• ProplydRelated: Winds from nearby massive stars can shape proplyd envelopes alongside ultraviolet radiation.

• R136Related: Powerful winds from R136’s massive stars remove mass and shape the surrounding nebula.

• Rosette NebulaRelated: Winds from massive cluster stars help clear gas from the nebula’s center.

• Stellar astronomyRelated: Winds remove mass and energy, changing stellar evolution and enriching nearby material.

• SupergiantRelated: Powerful winds strip mass from many supergiants and alter their later evolution.

• Herbig Ae/Be starRelated: Radiation and magnetic processes drive mass loss from young A- and B-type stars.

• Local BubbleRelated: Winds from massive stars can help clear and heat gas before they explode.

• Circumstellar discCompared with: Winds carry material away from a star, while discs retain material in orbit.

• Dumbbell NebulaRelated: Stellar winds help shape the material surrounding the star that produced the nebula.

• HypergiantRelated: Hypergiant winds carry away substantial mass and alter the star's evolution.

• NGC 6302Related: Fast stellar outflows help shape the nebula’s expanding lobes.

• Trapezium ClusterRelated: Winds from massive members help clear and compress gas around the young cluster.

• UY ScutiRelated: A strong wind carries material away from UY Scuti’s extended atmosphere.

• CW LeonisRelated: The slow, dense wind carries CW Leonis’s material into its expanding envelope.

• Epsilon Canis MajorisRelated: Adhara’s hot primary drives a strong outflow into surrounding space.

• LBV 1806−20Related: A strong wind carries mass away from LBV 1806−20 and shapes its circumstellar environment.

• NGC 7027Related: The central star's fast wind reshapes the nebula's earlier, slower ejecta.

• Zeta OphiuchiRelated: The wind collides with interstellar material to produce the star's bow shock.