by neufer » Thu Mar 06, 2008 10:33 pm
I would think that, like the Pencil Nebula, that is just another piece of the Vela Supernova:
http://violet.pha.jhu.edu/%7Ewpb/hstvela/hstvela.html
OTOH, it might also be generated by a Wolf-Rayet star in Gamma Velorum (or 'Regor'
).
http://antwrp.gsfc.nasa.gov/apod/ap060519.html
http://antwrp.gsfc.nasa.gov/apod/ap080117.html
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http://en.wikipedia.org/wiki/Gamma_Velorum
http://en.wikipedia.org/wiki/Wolf-Rayet_star
<<Wolf-Rayet stars (often referred to as WR stars) are evolved, massive stars (over 20 solar masses), and are losing their mass rapidly by means of a very strong stellar wind, with speeds up to 2000 km/s. While our own sun loses 10−16 of its own mass every year, a Wolf-Rayet star loses 10−5 solar masses a year. These stars are also very hot: their surface temperatures are in the range of 25,000 K to 50,000 K. The best known (and most visible) example of a Wolf-Rayet star is Gamma 2 Velorum (γ² Vel), which is a bright star visible to those located south of 40 degrees northern latitude. One of the members of the star system (Gamma Velorum is actually at least six stars) is a Wolf-Rayet star. Due to the exotic nature of its spectrum (bright emission lines in lieu of dark absorption lines) it is dubbed the "Spectral Gem of Southern Skies".>>
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Which do you think?
[quote="orin stepanek"]http://apod.nasa.gov/apod/ap080306.html
OK; I see it! :) Thanks neufer. What is the straight line of light above the bright blue star?[/quote]
I would think that, like the Pencil Nebula, that is just another piece of the Vela Supernova:
http://violet.pha.jhu.edu/%7Ewpb/hstvela/hstvela.html
OTOH, it might also be generated by a Wolf-Rayet star in Gamma Velorum (or 'Regor' :wink:).
http://antwrp.gsfc.nasa.gov/apod/ap060519.html
http://antwrp.gsfc.nasa.gov/apod/ap080117.html
--------------------------------------------
http://en.wikipedia.org/wiki/Gamma_Velorum
http://en.wikipedia.org/wiki/Wolf-Rayet_star
<<Wolf-Rayet stars (often referred to as WR stars) are evolved, massive stars (over 20 solar masses), and are losing their mass rapidly by means of a very strong stellar wind, with speeds up to 2000 km/s. While our own sun loses 10−16 of its own mass every year, a Wolf-Rayet star loses 10−5 solar masses a year. These stars are also very hot: their surface temperatures are in the range of 25,000 K to 50,000 K. The best known (and most visible) example of a Wolf-Rayet star is Gamma 2 Velorum (γ² Vel), which is a bright star visible to those located south of 40 degrees northern latitude. One of the members of the star system (Gamma Velorum is actually at least six stars) is a Wolf-Rayet star. Due to the exotic nature of its spectrum (bright emission lines in lieu of dark absorption lines) it is dubbed the "Spectral Gem of Southern Skies".>>
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Which do you think?