Abstract
The correctness of any theory rests with the lack of mathematical or numerical errors, so that its conclusions would follow from its assumptions and known physical laws. A correct theory, however, can be irrelevant unless its assumptions are consistent with observations or experiments. It is therefore essential that the physical properties of star-forming interstellar clouds be understood quantitatively before a theory of star formation becomes both correct and relevant.
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Mouschovias, T.C., Ciolek, G.E. (1999). Magnetic Fields and Star Formation: A Theory Reaching Adulthood. In: Lada, C.J., Kylafis, N.D. (eds) The Origin of Stars and Planetary Systems. NATO Science Series, vol 540. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-4509-1_9
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