Stable Hydrogen-burning Limits in Rapidly Rotating Very Low Mass Objects

We present novel effects of uniform rapid stellar rotation on the minimum mass stable hydrogen burning in very low stars, using an analytic model, and relaxing assumption spherical symmetry. obtain formula for as a function angular speed rotation. Further, we show existence maximum such which is purely artefact The this extremum results admissible value period $\sim 22$ min, below object does not reach main sequence, within ambits our model. For given speed, predict range beyond will evolve into sequence star.