Open AccessStar Formation, Using Three-Dimensional Explicit Eulerian Hydrodynamics.
Author(s) -
H. A. Williams
Publication year - 1988
Language(s) - Uncategorized
Resource type - Dissertations/theses
DOI - 10.31390/gradschool_disstheses.4549
Subject(s) - physics , angular momentum , instability , rotational symmetry , protostar , mechanics , neutron star , classical mechanics , gravitation , star formation , compact star , gravitational potential , compressibility , astrophysics , stars
Accelerating Research
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom
Address
John Eccles HouseRobert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom