title   
  

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

Güver, Tolga and Özel, Feryal (2013) The mass and the radius of the neutron star in the transient low mass X-ray binary SAX J1748.9−2021. Astrophysical Journal Letters, 765 (1). ISSN 2041-8205 (Print) 2041-8213 (Online)

This is the latest version of this item.

[img]
Preview
PDF (This is a RoMEO green journal -- author can archive pre-print (ie pre-refereeing) and post-print (ie final draft post-refereeing)) - Requires a PDF viewer such as GSview, Xpdf or Adobe Acrobat Reader
129Kb

Official URL: http://dx.doi.org/10.1088/2041-8205/765/1/L1

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 the Rossi X-ray Timing Explorer 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-circle dot or R = 10.93 +/- 2.09 km and M = 1.33 +/- 0.33 M-circle dot.

Item Type:Article
Additional Information:Article Number: L1
Uncontrolled Keywords:stars: neutron; X-rays: binaries; X-rays: individual (SAX J1748-2021)
Subjects:Q Science > QB Astronomy
Q Science > QC Physics
ID Code:25207
Deposited By:Tolga Güver
Deposited On:19 Nov 2014 16:03
Last Modified:19 Nov 2014 16:03

Available Versions of this Item

Repository Staff Only: item control page