* موقع الكون في الإنترنت* physics.usyd.edu.au Some Wolf–Rayet stars in binaries are close enough that we can image a rotating "pinwheel nebula" showing the dust generated by colliding winds in the binary system, from Aperture Masking Interferometry observations.
== See also ==* Gamma-ray burst* Hypernova* Starburst galaxy* Wolf–Rayet nebula* WR 104== References ==== External links ==* physics.usyd.edu.au Some Wolf–Rayet stars in binaries are close enough that we can image a rotating "pinwheel nebula" showing the dust generated by colliding winds in the binary system, from Aperture Masking Interferometry observations.