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The Radcliffe wave is a neighbouring coherent gaseous structure in the Milky Way, dotted with a related high concentration of interconnected stellar nurseries. It stretches about 8,800 light years. This structure runs with the trajectory of the Milky Way arms.
Movements, Structure and movement & Discovery
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| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| Radcliffe wave | is a | neighbouring coherent gaseous structure in the Milky Way | 0.90 | text |
| Monoceros OB1 | instance of | The latter is more dispersed as to its interstellar medium than the wave and has further large star-forming regions | 0.80 | text |
| California Nebula | instance of | The latter is more dispersed as to its interstellar medium than the wave and has further large star-forming regions | 0.80 | text |
| Cepheus Far | instance of | The latter is more dispersed as to its interstellar medium than the wave and has further large star-forming regions | 0.80 | text |
| and Rho Ophiuchi.A 2024 paper announced the discovery that the Radcliffe wave is oscillating in the form of a traveling wave | instance of | The latter is more dispersed as to its interstellar medium than the wave and has further large star-forming regions | 0.80 | text |
| Radcliffe wave | related to External links | Interactive | 0.60 | section |
| Radcliffe wave | related to External links | Radcliffe | 0.60 | section |
| Radcliffe wave | related to External links | Harvard University | 0.60 | section |
| Radcliffe wave | related to Formation | Scientists | 0.60 | section |
| Radcliffe wave | related to Formation | It | 0.60 | section |
| Radcliffe wave | related to Formation | Milky Way | 0.60 | section |
| Radcliffe wave | related to Formation | Inside | 0.60 | section |
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