SIMBAD references

1994A&AS..108..455S - Astron. Astrophys., Suppl. Ser., 108, 455-459 (1994/December-1)

High precision rotating neutron star models. II. Large sample of neutron star properties.

SALGADO M., BONAZZOLA S., GOURGOULHON E. and HAENSEL P.

Abstract (from CDS):

A new and highly precise numerical approach for computing stationary rotating stellar configurations in general relativity has been employed to construct rotating neutron star models. Fourteen equations of state (EOS) of cold dense matter have been used to produce a "catalog" of thousands neutron star models, parametrized by the EOS, the central energy density and the angular velocity. The results are presented in a series of tables for each EOS. A particular emphasis is put on the properties of maximal mass models. These latter are useful to constrain the EOS, taking into account the observed pulsars.

Abstract Copyright: ∼

Journal keyword(s): relativity - stars: neutron - rotation - pulsars - equations of state

VizieR on-line data: <Available at CDS (J/A+AS/108/455): tables tables.tex>

Simbad objects: 2

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