ผลต่างระหว่างรุ่นของ "ดาววอลฟ์–ราแย"

 

== แหล่งข้อมูลอื่น ==

* [http://www.physics.usyd.edu.au/~gekko/wr104.html 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.

* [http://cfa-www.harvard.edu/~pberlind/atlas/htmls/wrstars.html harvard.edu] Wolf–Rayet Stars: Spectral Classifications