Distribution of the Masses of Protostars in Globular Clusters

A technical analysis of the formation of globular clusters, that utilizes just gravity and the progression of the natural reference system to form stars and clusters. Discussed are the mass limits for stellar combustion, as well as radial separations.

International Society of  Unified Science
Reciprocal System Research Society

Salt Lake City, UT 84106
USA

Theme by Danetsoft and Danang Probo Sayekti inspired by Maksimer