WR 124 | is a part of Milky Way | ![2001-09-27 09:30:30.0 2001-09-27 09:30:30.0](facet.gif) |
has spectral type WN8 | ![2001-09-27 09:30:30.0 2001-09-27 09:30:30.0](facet.gif) |
has spectral type WN 8 | ![2001-09-27 09:30:30.0 2001-09-27 09:30:30.0](facet.gif) |
has distance 15000 light-years | ![2001-09-27 09:30:30.0 2001-09-27 09:30:30.0](facet.gif) |
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 URL: http://adsabs.harvard.edu/cgi-bin/bib_query?1999IAUS..193..356G, 2001-09-27 09:30:30.0 has URL: http://adsabs.harvard.edu/cgi-bin/bib_query?1999IAUS..193..356G, 2001-09-27 09:30:30.0](facet.gif) |
has image emission nebula M1-67
![](http://oposite.stsci.edu/pubinfo/pr/1998/38/content/9838x.jpg) | ![has URL: http://oposite.stsci.edu/pubinfo/pr/1998/38, 2001-09-27 09:30:30.0 has URL: http://oposite.stsci.edu/pubinfo/pr/1998/38, 2001-09-27 09:30:30.0](facet.gif) |
has velocity 200 km/s | ![2001-09-27 09:30:30.0 2001-09-27 09:30:30.0](facet.gif) |
is an instance of WN star | ![has URL: http://oposite.stsci.edu/pubinfo/pr/1998/38, 2001-09-27 09:30:30.0 has URL: http://oposite.stsci.edu/pubinfo/pr/1998/38, 2001-09-27 09:30:30.0](facet.gif) |
WN star | has emission line He I, He II, N III, N IV or N V | ![2001-09-27 09:30:30.0 2001-09-27 09:30:30.0](facet.gif) |
Wolf-Rayet | has ejection velocity 2000 km s-1 | ![2001-09-27 09:30:30.0 2001-09-27 09:30:30.0](facet.gif) |
has temperature up to 50000 K | ![2001-09-27 09:30:30.0 2001-09-27 09:30:30.0](facet.gif) |
star | has star surface temperature | ![2001-09-27 09:30:25.0 2001-09-27 09:30:25.0](facet.gif) |
has V magnitude | ![2001-09-27 09:30:25.0 2001-09-27 09:30:25.0](facet.gif) |
has B magnitude | ![2001-09-27 09:30:25.0 2001-09-27 09:30:25.0](facet.gif) |
has U magnitude | ![2001-09-27 09:30:25.0 2001-09-27 09:30:25.0](facet.gif) |
has position on celestial sphere from the point of view of Earth | ![2001-09-27 09:30:25.0 2001-09-27 09:30:25.0](facet.gif) |
has parallax from the point of view of Earth's orbit | ![2001-09-27 09:30:25.0 2001-09-27 09:30:25.0](facet.gif) |
has proper motion | ![2001-09-27 09:30:24.0 2001-09-27 09:30:24.0](facet.gif) |
has radiation at surface which is diffused out from the hotter core | ![2001-09-27 09:30:24.0 2001-09-27 09:30:24.0](facet.gif) |
has energy source gravitational contraction and or fusion | ![2001-09-27 09:30:24.0 2001-09-27 09:30:24.0](facet.gif) |
has energy production which takes place primarily within the core | ![2001-09-27 09:30:24.0 2001-09-27 09:30:24.0](facet.gif) |
has surface density which depends on luminosity class | ![2001-09-27 09:30:24.0 2001-09-27 09:30:24.0](facet.gif) |
has surface temperature greater than 1000 Kelvin | ![2001-09-27 09:30:24.0 2001-09-27 09:30:24.0](facet.gif) |
has apparent magnitude | ![2001-09-27 09:30:25.0 2001-09-27 09:30:25.0](facet.gif) |
has absolute magnitude | ![2001-09-27 09:30:25.0 2001-09-27 09:30:25.0](facet.gif) |
has age | ![2001-09-27 09:30:25.0 2001-09-27 09:30:25.0](facet.gif) |
has catalog star catalog | ![2001-09-27 09:30:25.0 2001-09-27 09:30:25.0](facet.gif) |
has material hydrogen, helium | ![2001-09-27 09:30:24.0 2001-09-27 09:30:24.0](facet.gif) |
has mass greater than 0.08 the sun's mass | ![2001-09-27 09:30:24.0 2001-09-27 09:30:24.0](facet.gif) |
celestial body | has spectra | ![2001-09-27 09:30:09.0 2001-09-27 09:30:09.0](facet.gif) |
physical object | has location or center of gravity | ![2001-09-27 09:27:27.0 2001-09-27 09:27:27.0](facet.gif) |
has angular momentum | ![2001-09-27 09:27:27.0 2001-09-27 09:27:27.0](facet.gif) |
has momentum | ![2001-09-27 09:27:27.0 2001-09-27 09:27:27.0](facet.gif) |
has volume | ![2001-09-27 09:27:27.0 2001-09-27 09:27:27.0](facet.gif) |
has extent | ![2001-09-27 09:27:27.0 2001-09-27 09:27:27.0](facet.gif) |