Top Results for Dust Spiral
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LL Pegasi is a carbon-rich star within a prominent spiral nebula. This young, protoplanetary nebula formed due to continuous mass ejection from a binary star system. The resulting structure, characterized by distinct dust rings, offers astronomers a unique opportunity to study the processes of stell...
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WR 140 is a variable star system located in the constellation Cygnus, consisting of a massive Wolf-Rayet star and a hot O-type giant companion. These two stars follow a highly eccentric 7.9-year orbit, coming close enough together to generate colliding stellar winds that shock the surrounding gas. T...
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Colliding-wind binary with periodic dust shells, strong specialist and JWST-era visibility.
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