Open AccessStar Formation, Using Three-Dimensional Explicit Eulerian Hydrodynamics.
Author(s) -
Harold A. Williams
Publication year - 2022
Language(s) - Uncategorized
Resource type - Dissertations/theses
DOI - 10.31390/gradschool_disstheses.4549
Subject(s) - physics , angular momentum , instability , rotational symmetry , protostar , classical mechanics , mechanics , neutron star , gravitation , star formation , gravitational potential , compact star , astrophysics , stars