Could anyone clearly demonstrate how rotation and turbulence exactly affect self-gravitational collapse dynamics to structure formation out of molecular clouds?
Quantitative and directional analyses in comparison with the gravitational ones would be highly appreciated in this clear context of bounded structure formation.
Patrick Okezuonu
From Jean's law, a particular amount of cloud mass is needed to trigger gravitational collapse of star/structure formation but due to the rotational motion as can be caused by turbulence forces, emerging from the clouds environment prevent the accumulation of more masses to cause collapse or even reduces the already accumulated masses thereby causing delay in star/structure formation.
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