Cosmology
The Milky Way warp refers to the bending or distortion of the galactic disk of the Milky Way galaxy, particularly in its outer regions. This phenomenon is thought to arise due to gravitational influences from nearby structures, such as satellite galaxies and dark matter, leading to a misalignment of the galaxy's plane with respect to the surrounding universe. Understanding the warp provides insights into the dynamics and formation processes of galaxies, connecting it to broader galaxy formation theories and models.
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