| 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 |  |