The mass and the radius of the neutron star in the transient low mass X-ray binary SAX J1748.9-2021

TL;DR

This study estimates the neutron star's mass and radius in SAX J1748.9-2021 using time-resolved X-ray burst spectroscopy, providing two possible solutions consistent with observational data.

Contribution

The paper introduces a method combining burst spectroscopy and distance measurements to constrain neutron star properties in a specific binary system.

Findings

Two possible neutron star mass-radius solutions identified.

Measured radius ranges from approximately 8.2 to 10.9 km.

Mass estimates range from about 1.33 to 1.78 solar masses.

Abstract

We use time resolved spectroscopy of thermonuclear X-ray bursts observed from SAX J1748.9-2021 to infer the mass and the radius of the neutron star in the binary. Four X-ray bursts observed from the source with RXTE enable us to measure the angular size and the Eddington limit on the neutron star surface. Combined with a distance measurement to the globular cluster NGC 6440, in which SAX J1748.9-2021 resides, we obtain two solutions for the neutron star radius and mass, R = 8.18 +/- 1.62 km and M = 1.78 +/- 0.3 M_\sun or R = 10.93 +/- 2.09 km and M = 1.33 +/- 0.33 M_\sun.