The Distance, Mass, and Radius of the Neutron Star in 4U 1608-52

Details The Distance, Mass, and Radius of the Neutron Star in 4U 1608-52 The Distance, Mass, and Radius of the Neutron Star in 4U 1608-52

2008-11-25

arxiv.org/abs/0811.3979v4

Astrophys.J.712:964-973, 2010

Astronomy and Astrophysics

Astrophysics

ApJ in print. Resulting probability distributions of our measurements can be found at http://ice.as.arizona.edu/~ns

Scientific paper

10.1088/0004-637X/712/2/964

Low mass X-ray binaries that show thermonuclear bursts are ideal sources for constraining the equation of state of neutron star matter. The lack of independent distance measurements for most of these sources, however, prevents a systematic exploration of the masses and radii of the neutron stars, hence limiting the equation of state studies. We present here a measurement of the distance to the low mass X-ray binary 4U 1608-52 that is based on the study of the interstellar extinction towards the source. We first model the individual absorption edges of the elements Ne and Mg in the high resolution X-ray spectrum obtained with XMM-Newton. We then combine this information with a measurement of the run of reddening with distance using red clump stars and determine a minimum distance to the source of 3.9 kpc, with a most probable value of 5.8 kpc. Finally, we analyze time-resolved X-ray spectra of Type-I X-ray bursts observed from this source to measure the mass and the radius of the neutron star. We find a mass of M = 1.74 +/- 0.14 M_sun and a radius of R = 9.3 +/- 1.0 km, respectively. This mass and radius can be achieved by several multi-nucleon equations of state.

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