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Star Formation in Magnetized, Turbulent and Rotating Molecular Cloud: The Critical Mass

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Figure

Figure 2. When magnetic field lines stretched over its radius of curvature. Here, the
Figure 3. The pre-stellar core radius vs its relative critical mass (MC radius Mcrt). Assuming parent R1 pco =, Ω1013s1core−−, R0.01 pc - 0.1 pccore=, c332 m s1s=⋅−,  ρ1010kg m3core=−⋅−, and σ400 m s1r=⋅−
Figure 4. Critical mass comparison of unmagnetized and magnetized, but rotating and turbulent MC core
Figure 6. Critical mass comparison of non-turbulent and non-rotating, but magnetized MCc (the black curve) with turbulent and rotating magnetized MCc (the blue curve)
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