KnowraMassive starLinked fromLinked fromThe 17 pages that link to Massive star, each with the reason it gives.All 17Broader topic 2Related 4Narrower topic 9Compared with 2Core-collapse supernovaNarrower topic: Only stars above a threshold initial mass generally reach the advanced burning stages that lead to this event.Wolf–Rayet starNarrower topic: Most Wolf–Rayet stars are understood as evolved massive stars that have shed much of their mass.Eta CarinaeNarrower topic: Eta Carinae demonstrates how extreme mass loss can alter a massive star before its final fate.Pair-instability supernovaNarrower topic: Pair-instability progenitors begin as massive stars capable of building large oxygen-rich cores.Luminous blue variableNarrower topic: The class consists of evolved stars from the high-mass end of stellar populations.R136Narrower topic: R136’s most distinctive members belong to this short-lived, energetic stellar class.Trapezium ClusterNarrower topic: The cluster offers a close setting for examining massive stars and their effects.Beta CentauriNarrower topic: The system’s bright components belong to the hot, high-mass stellar population.Yellow supergiantNarrower topic: Many yellow supergiants descend from massive stars after leaving the main sequence.