KnowraWolf–Rayet starLinked fromLinked fromThe 20 pages that link to Wolf–Rayet star, each with the reason it gives.All 20Broader topic 2Related 11Compared with 7Stellar windRelated: Its powerful wind can remove much of the star’s outer layers.Williamina FlemingRelated: Fleming identified the unusual spectrum of the star later known as Wolf–Rayet.Cassiopeia ARelated: Cassiopeia A’s progenitor likely shed most of its hydrogen before exploding.Cosmic dustRelated: Some Wolf–Rayet systems create dust where colliding stellar winds compress and cool.Pair-instability supernovaRelated: Some proposed pair-instability progenitors reach the required core conditions after losing their outer layers.Tarantula NebulaRelated: The nebula contains such stars, whose winds reveal late stages of massive-star evolution.Triangulum GalaxyRelated: M33 contains observed Wolf–Rayet stars that trace massive-star evolution.Blue supergiantRelated: Mass loss can strip a blue supergiant’s envelope and lead toward a Wolf–Rayet phase.R136Related: Several exceptionally massive stars associated with R136 have Wolf–Rayet characteristics.HypernovaRelated: Stripped massive stars are leading candidates for long-burst hypernova progenitors.Type Ib and Ic supernovaeRelated: Some proposed progenitors are stripped Wolf–Rayet stars, though binary stars can also produce them.