Constraints on the mass and radius of neutron stars from X-ray observations
arXiv:1512.06991
Abstract
This article gives a very brief introduction about measuring the mass and radius of neutron star from X-ray observations. The masses and radii of neutron stars can be determined from photospheric radius expansion bursts in low-mass X-ray binaries, X-ray pulse profile modeling in accreting X-ray pulsars, gravitational redshift measurement in low-mass X-ray binaries and thermal X-ray spectral fitting in quiescent low-mass X-ray binaries.
3 pages, 1 figure. Proceeding of "Quarks and Compact Stars 2014 at KIAA (Beijing)"