A two-component model combining self-gravity and galactic shear reproduces the steep velocity dispersion-size relation of molecular clouds and its radial variation across the Milky Way.
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Shear-gravity transition determines the steep velocity dispersion-size relation in molecular clouds: confronting analytical formula with observations
A two-component model combining self-gravity and galactic shear reproduces the steep velocity dispersion-size relation of molecular clouds and its radial variation across the Milky Way.