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- W33365626 abstract "Results are outlined of a submillimetre study of pre-stellar cores. The pre-stellar phase is one in which a dense core in a molecular cloud is gravitationally bound, but contains no embedded luminosity source. This takes place prior to the protostellar Class 0 phase, which is the main infall phase of star formation. The observations of pre-stellar cores are compared to different models of star formation. The radial density profiles are inconsistent with a singular isothermal sphere but consistent with predictions of a magnetic support model, indicating that the cores are undergoing ambipolar diffusion prior to the main protostellar collapse phase." @default.
- W33365626 created "2016-06-24" @default.
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- W33365626 date "1996-01-01" @default.
- W33365626 modified "2023-09-27" @default.
- W33365626 title "New Millimetre Observations of Pre-stellar Cores" @default.
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- W33365626 doi "https://doi.org/10.1007/978-3-540-68594-4_20" @default.
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