The giant in our stars

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The Radcliffe wave is a huge gaseous structure within the Milky Way where stars
The Radcliffe wave is a huge gaseous structure within the Milky Way where stars form (© Alyssa Goodman/Harvard University).
The Radcliffe wave is a huge gaseous structure within the Milky Way where stars form (© Alyssa Goodman/Harvard University). Interconnected stellar nurseries form the largest gaseous structure ever observed in the Milky Way galaxy. Astronomers of the University of Vienna and Harvard University have discovered a monolithic, wave-shaped gaseous structure - the largest ever seen in our galaxy - made up of interconnected stellar nurseries. Dubbed the "Radcliffe wave" in honor of the collaboration's home base, the discovery transforms a 150-year-old vision of nearby stellar nurseries as an expanding ring into one featuring an undulating, star-forming filament that reaches trillions of miles above and below the galactic disk. The work launched in 2013 with the mission of precisely measuring the position, distance, and motion of the stars. The research team combined the super-accurate data from Gaia with other measurements to construct a detailed, 3-D map of interstellar matter in the Milky Way, and noticed an unexpected pattern in the spiral arm closest to the Earth. The researchers discovered a long, thin structure, about 9,000 light years long and 400 light years wide, with a wave-like shape, cresting 500 light years above and below the mid-plane of our Galaxy's disk.
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