摘要
We present a new method for determining masses and radii of neutron stars residing in thermonuclear X-ray burst sources. To illustrate this method, we apply it to a burst from the source 4U 1820-30 recorded by the Rossi X-Ray Timing Explorer. Fits of the observed X-ray spectra to grids of Comptonized model atmospheres yield estimates for the mass and radius of the neutron star, M = 1.3 +/- 0.6 M-circle dot and R = 11(-2)(+3) km, respectively.
- 出版日期2011-8