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Infalling motions were detected and modeled toward this source. A mean infallvelocity of 0.5 km/s with an infall mass rate of 5x10^-3 Solar masses per yearwas obtained. Also, a previously estimated value for the magnetic fieldstrength in the plane of the sky was refined to be 855 micro Gauss which weused to calculate a mass-to-magnetic flux ratio of 1.9, or super-critical. Thevirial mass from turbulent motions was also calculated finding Mvir=563 solarmasses, which gives a ratio of Msubmm/Mvir=5.9. Both values strongly suggestthat this clump must be in a state of gravitational collapse.

G30.79~FIR~10: A gravitationally bound infalling high-Mass star forming clump