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 | |