Hartland Snyder and J. Robert Oppenheimer calculated the gravitational collapse of an idealized, spherical, pressureless star. The Oppenheimer-Snyder model connects a comoving dust interior with a vacuum exterior and follows contraction beyond the limits of a static stellar model.[ref]
On Continued Gravitational Contraction by J. Robert Oppenheimer and Hartland Snyder. 1939 spherical-collapse calculation and distant/comoving time descriptions