Linked from

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

• Stellar evolutionRelated: Mass loss through winds can alter a star’s later stages and final remnant.

• Interstellar mediumRelated: Stellar winds inject energy and material into surrounding interstellar gas.

• Planetary nebulaRelated: A slow, dense wind builds the material later shaped into the nebula.

• Stellar feedbackRelated: Winds carry momentum and energy from massive stars into nearby gas before they explode.

• Stellar atmosphereRelated: Atmospheric material can escape into space as a stellar wind.

• Asymptotic giant branchRelated: A dense wind removes the envelope and helps end the branch phase.

• Wolf–Rayet starRelated: Radiation pressure on spectral lines drives the dense outflows that shape Wolf–Rayet spectra.

• Ultraviolet astronomyRelated: Ultraviolet spectral lines reveal wind speeds and mass loss from hot stars.

• Orion NebulaRelated: Winds from massive young stars help sculpt cavities and fronts in the gas.

• Stellar radiusRelated: Outflowing material can extend beyond the photosphere without defining the photospheric radius.

• BetelgeuseRelated: Betelgeuse sheds material through a powerful wind that feeds its dusty surroundings.

• Massive starRelated: Strong winds from massive stars inject momentum and enriched material into the interstellar medium.

• Emission nebulaRelated: Winds from massive stars carve cavities and compress gas around emission nebulae.

• Herbig–Haro objectRelated: Winds can shape the surroundings, but Herbig–Haro knots trace collimated jet impacts.

• Red supergiantRelated: Red supergiants shed substantial material through slow, dense winds.

• Cygnus X-1Related: The black hole captures part of the companion’s powerful stellar wind.

• Galactic windRelated: Winds from massive stars add momentum and energy before those stars explode.

• Proxima CentauriRelated: Proxima’s wind can interact strongly with the atmospheres and magnetospheres of close planets.

• T Tauri starRelated: Outflows remove angular momentum and compete with accretion for circumstellar material.

• Stellar activityRelated: It is a persistent consequence of atmospheric processes, unlike many short-lived activity events.

• Carina NebulaRelated: Winds from massive stars carve cavities and compress gas within the nebula.

• AntaresRelated: Antares sheds material through a wind that helps shape its circumstellar environment.

• Carbon starRelated: Carbon stars shed enriched atmospheres through strong winds, returning carbon and dust to space.

• Circumstellar envelopeRelated: It carries much of the material that builds an envelope around an evolving star.

• Debris diskRelated: For active stars, wind drag can remove dust alongside radiation-driven forces.

• O-type starRelated: Intense radiation drives powerful winds that remove mass from O-type stars.

• Circumstellar mediumRelated: It carries stellar material outward and helps set the medium’s density and shape.

• Eagle NebulaRelated: Winds from young massive stars help sculpt the nebula’s gas and dust.

• Horsehead NebulaRelated: Winds from nearby massive stars contribute to sculpting the cloud's exposed face.

• Pair-instability supernovaRelated: Uncertain mass loss changes whether a star retains the core mass needed for pair instability.

• Proxima Centauri bRelated: A strong stellar wind could erode Proxima Centauri b’s atmosphere over time.

• Ring NebulaRelated: Winds from the progenitor and its exposed core shaped the surrounding nebular gas.

• Tarantula NebulaRelated: Winds from its massive stars inject momentum and energy into surrounding gas.

• MiraRelated: Mira’s wind carries material away from its pulsating atmosphere.

• Population II starRelated: Winds from earlier stars also returned newly made elements to star-forming gas.

• Stellar coronaRelated: Coronal plasma expands outward and supplies much of a star’s wind.

• Stellar magnetic fieldRelated: Magnetic fields shape the wind and help stars shed angular momentum.

• Blue supergiantRelated: Intense radiation drives strong winds that remove mass from blue supergiants.

• Cat's Eye NebulaRelated: Winds from the central star interact with older expelled gas to sculpt the nebula's shells.

• RigelRelated: Rigel loses material through a strong wind driven by its intense radiation.

• Pillars of CreationRelated: Winds from young massive stars help sculpt and disperse the surrounding gas.

• VY Canis MajorisRelated: A dense outflow carries gas away from the star and shapes its surrounding nebula.

• DenebRelated: Deneb loses material through a strong wind driven by its luminous atmosphere.

• Giant starRelated: Strong winds from evolved giants can remove much of their outer envelopes.

• Lagoon NebulaRelated: Winds from massive stars excavate cavities and compress gas within the nebula.

• 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.