Linked from

The 26 pages that link to Stellar feedback, each with the reason it gives.

• Star formationRelated: Feedback from newly formed stars can disperse clouds or trigger further collapse.

• Initial mass functionRelated: The distribution sets how many energetic massive stars inject feedback into a population's environment.

• Starburst galaxyRelated: Feedback can disrupt star-forming clouds or drive gas out, limiting a burst.

• Galaxy evolutionRelated: Winds and supernovae regulate how efficiently gas becomes stars.

• Galaxy formation and evolutionRelated: It regulates star formation and can drive gas out of galaxies.

• ReionizationRelated: Feedback can open channels through which ionizing photons escape small early galaxies.

• Massive starRelated: Radiation and outflows from forming massive stars can impede further accretion and reshape their birth clouds.

• Dwarf galaxyRelated: Supernovae and stellar winds can expel gas from shallow dwarf-galaxy gravitational wells.

• Stellar associationRelated: Feedback can expel gas and leave a young stellar grouping gravitationally unbound.

• O-type starRelated: O-star radiation and winds can disperse natal clouds and regulate further star formation.

• Star formation efficiencyRelated: Feedback can disperse star-forming gas and limit its conversion into stars.

• Tarantula NebulaRelated: Winds and radiation from massive stars reshape the nebula and regulate further star formation.

• Too-big-to-fail problemRelated: It can alter dwarf-galaxy formation and the central densities inferred from their stars.

• Flocculent spiral galaxyRelated: Feedback may disperse star-forming regions and alter the persistence of visible arm segments.

• R136Related: R136’s winds and radiation alter the nebula and influence later star formation.

• Super star clusterRelated: Feedback clears natal gas and can determine whether a young cluster survives.

• Interstellar cloudRelated: New stars can heat, disperse, or compress the clouds that formed them.

• Omega NebulaRelated: Radiation and winds from young massive stars sculpt the surrounding gas.

• Formation and evolution of stars and galaxiesRelated: Feedback can halt star formation locally while regulating gas across a galaxy.

• Starburst regionRelated: Feedback can heat or expel gas, limiting a starburst’s duration.

• Stochastic self-propagating star formation modelRelated: Feedback from young stars can compress neighboring gas and trigger another episode.

• Westerhout 40Related: Radiation and winds from massive stars alter the clouds around Westerhout 40.