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 |  |