X-ray observations of neutron stars and the equation of state at supra-nuclear densities

Details X-ray observations of neutron stars and the equation of state at supra-nuclear densities X-ray observations of neutron stars and the equation of state at supra-nuclear densities

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010newar..54..122t&link_type=abstract

New Astronomy Reviews, Volume 54, Issue 3-6, p. 122-127.

Astronomy and Astrophysics

Astronomy

Scientific paper

This article summarizes recent progress which has been made in
constraining the equation of state of nuclear matter at supra-nuclear
densities by X-ray observations of neutron stars. The main conclusion is
that the equation of state is rather stiff.

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