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• W3099185810 startingPage "579" @default.
• W3099185810 abstract "The dense molecular cloud cores that form stars, like other self-gravitating objects, undergo bulk oscillations. Just at the point of gravitational instability, their fundamental oscillation mode has zero frequency. We study, using perturbation theory, the evolution of a spherical cloud that possesses such a frozen mode. We find that the cloud undergoes a prolonged epoch of subsonic, accelerating contraction. This slow contraction occurs whether the cloud is initially inflated or compressed by the oscillation. The subsonic motion described here could underlie the spectral infall signature observed in many starless dense cores." @default.
• W3099185810 created "2020-11-23" @default.
• W3099185810 creator A5001758552 @default.
• W3099185810 creator A5087117873 @default.
• W3099185810 date "2009-06-11" @default.
• W3099185810 modified "2023-09-27" @default.
• W3099185810 title "The approach to collapse of molecular clouds" @default.
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• W3099185810 doi "https://doi.org/10.1111/j.1365-2966.2009.14737.x" @default.
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