Abstract
view Abstract Citations (684) References (11) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Slowly Rotating Relativistic Stars. II. Models for Neutron Stars and Supermassive Stars Hartle, James B. ; Thorne, Kip S. Abstract The equilibrium configurations of rigidly rotating white dwarfs and neutron stars are calculated using the Harrison-Wheeler and the Tsuruta-Cameron V1 equations of state, along with the general-relativistic equations of structure. The equations of structure used are the exact relativistic equations with one ex- ception: they have been expanded in powers of the angular velocity ~2, and terms of higher order than ~ have been neglected. The equilibrium configurations of slowly rotating supermassive stars are also calculated Publication: The Astrophysical Journal Pub Date: September 1968 DOI: 10.1086/149707 Bibcode: 1968ApJ...153..807H full text sources ADS | Related Materials (7) Part 1: 1967ApJ...150.1005H Part 3: 1969ApJ...158..719H Part 4: 1975ApJ...195..203H Part 5: 1970ApJ...161..111H Part 6: 1975ApJ...198..467H Part 7: 1972ApJ...176..177H Part 8: 1975ApJ...196..653H
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