Wolf–Rayet stars

E290082

Wolf–Rayet stars are extremely hot, massive, and luminous evolved stars characterized by powerful stellar winds and strong emission lines from heavy elements in their spectra.

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All labels observed (1)

Label Occurrences
Wolf–Rayet stars canonical 3

Statements (50)

Predicate Object
instanceOf evolved star
massive star
stellar object
canBeProgenitorOf Type Ib supernova
Type Ic supernova
long gamma-ray burst
canProduce strong X-ray emission in binaries
discoveredAt Paris Observatory
discoveredIn 1867
evolutionaryStage core helium-burning phase
post-main-sequence
hasMassLossRate 10^-5 to 10^-4 solar masses per year
hasPopulation Population I star
hasStellarWind powerful stellar wind
hasSubtype WC star
WN star
WO star
hasTerminalWindVelocity 1000 to 5000 km/s
location Large Magellanic Cloud
Milky Way
surface form: Milky Way galaxy

Small Magellanic Cloud
metallicityDependence more common at high metallicity
namedAfter Charles Wolf
Georges Rayet
occursIn spiral arms of galaxies
star-forming regions
starburst galaxies
oftenInBinarySystemWith O-type star
massive companion star
progenitorType O-type star
roleInGalaxies source of chemical enrichment
source of ionizing radiation
source of mechanical feedback
spectralCharacteristic broad emission lines
lines of carbon
lines of helium
lines of nitrogen
lines of oxygen
strong emission lines
spectralClassSystem WN WC WO classification
surfaceComposition enriched in heavy elements
helium-rich
hydrogen-poor
typicalEffectiveTemperature 30000 to 200000 K
typicalLuminosity 10^5 to 10^6 times solar luminosity
typicalMass greater than 20 solar masses
variability often photometrically variable
WC star carbon-sequence Wolf–Rayet star
WN star nitrogen-sequence Wolf–Rayet star
WO star oxygen-sequence Wolf–Rayet star

Referenced by (3)

Full triples — surface form annotated when it differs from this entity's canonical label.

Carina Nebula contains Wolf–Rayet stars
IC 10 contains Wolf–Rayet stars
Tarantula Nebula ionizedBy Wolf–Rayet stars