KnowraSubrahmanyan ChandrasekharLinked fromLinked fromThe 9 pages that link to Subrahmanyan Chandrasekhar, each with the reason it gives.All 9Related 9Black holeRelated: His work clarified how stellar remnants can progress toward gravitational collapse.Dynamical frictionRelated: His 1943 analysis derived the standard estimate for drag from a distribution of field stars.AstrophysicsRelated: His mass limit clarified why stars end in different compact remnants.Arthur EddingtonRelated: Eddington publicly challenged Chandrasekhar’s theory of stellar collapse in the 1930s.Chandrasekhar limitRelated: His 1930s calculations gave the limit its name and physical basis.Yerkes ObservatoryRelated: Chandrasekhar spent much of his career at the University of Chicago and held a close institutional connection to Yerkes.William Alfred FowlerRelated: His theoretical account of stars provided a broader context for Fowler’s nuclear studies.Stellar black holeRelated: His limit clarified how massive stellar remnants can progress beyond white-dwarf support.Astronomical black holesRelated: His work clarified how stellar remnants can be driven toward further gravitational collapse.