| WR 124 | is a part of Milky Way |  | 
| has spectral type WN8 |  | 
| has spectral type WN 8 |  | 
| has distance 15000 light-years |  | 
| has reference Grosdidier, Y.; Moffat, A. F. J.; Blais-Ouellette, S.; Joncas, G.; Acker, A. : 1999, Proc. IAU Symp. 193, 356. M1-67, nebula ejected from the 200 km/s runaway WN8 star WR 124 |  | 
| has image emission nebula M1-67 
  |  | 
| has velocity 200 km/s |  | 
| is an instance of WN star |  | 
| WN star | has emission line He I, He II, N III, N IV or N V |  | 
| Wolf-Rayet | has ejection velocity 2000 km s-1 |  | 
| has temperature up to 50000 K |  | 
| star | has star surface temperature |  | 
| has V magnitude |  | 
| has B magnitude |  | 
| has U magnitude |  | 
| has position on celestial sphere from the point of view of Earth |  | 
| has parallax from the point of view of Earth's orbit |  | 
| has proper motion |  | 
| has radiation at surface which is diffused out from the hotter core |  | 
| has energy source gravitational contraction and or fusion |  | 
| has energy production which takes place primarily within the core |  | 
| has surface density which depends on luminosity class |  | 
| has surface temperature greater than 1000 Kelvin |  | 
| has apparent magnitude |  | 
| has absolute magnitude |  | 
| has age |  | 
| has catalog star catalog |  | 
| has material hydrogen, helium |  | 
| has mass greater than 0.08 the sun's mass |  | 
| celestial body | has spectra |  | 
| physical object | has location or center of gravity |  | 
| has angular momentum |  | 
| has momentum |  | 
| has volume |  | 
| has extent |  |