A Lack of Constraints on the Cold Opaque H I Mass: H I Spectra in M31 and M33 Prefer Multicomponent Models over a Single Cold Opaque Component
Monthly Notices of the Royal Astronomical Society（2021）
Key words
ISM: kinematics and dynamics,galaxies: individual: M33,galaxies: individual: M31,galaxies: ISM,radio lines: ISM
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