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to form much smaller and denser objects. As the gravitational collapse of an interstellar gas cloud is the first stage in the formation of a
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212:{\displaystyle M_{BE}(p_{0})={225 \over {32{\sqrt {5\pi }}}}{c_{s}^{4} \over {(aG)}^{3/2}}{1 \over {\sqrt {p_{0}}}}}
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which varies based on the density distribution of the cloud. For a uniform mass density
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gas sphere embedded in a pressurized medium can have while still remaining in
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545:. Oxfordshire United Kingdom: Princeton University Press. p.
40:, the Bonnor–Ebert mass is an important quantity in the study of
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Ebert, Rolf (1955). "Über die
Verdichtung von H I-Gebieten".
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409:{\displaystyle a\approx 1.67}
708:. You can help Knowledge by
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312:{\displaystyle \gamma =1}
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26:isothermal
401:≈
328:μ
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