Investigating Variability of Quiescent Neutron Stars in the Globular Clusters NGC 6440 and Terzan 5

Abstract

The quiescent spectrum of neutron star low-mass X-ray binaries typically consists of two components - a thermal component associated with emission from the neutron star surface, and a non-thermal power-law component whose origin is not well understood. Spectral fitting of neutron star atmosphere models to the thermal component is one of the leading methods for measuring the neutron star radius. However, it has been known for years that the X-ray spectra of quiescent neutron stars vary between observations. While most quiescent variability is explained through a variable power-law component, the brightest and best-studied object, Cen X-4, requires a change in the thermal component and such thermal variability could be a problem for measuring neutron star radii. In this paper, we significantly increase the number of sources whose quiescent spectra have been studied for variability. We examine 9 potential quiescent neutron stars with luminosities <1E34 erg/s over the course of multiple Chandra observations of the globular clusters NGC 6440 and Terzan 5 and find no strong evidence for variability in the effective temperature in 7 of the 9 sources. Two sources show a potential change in temperature, though this depends on the exact model fitted. CX1 in NGC 6440 is equally well fit by a variable thermal component or a variable power law. Therefore, the results are inconclusive and we cannot exclude or require thermal variability in that source. CX5 in NGC 6440 shows a potential change in temperature, though this depends on whether a power-law is included in the spectral fit or not. This suggests that thermal variability may not be widespread among quiescent neutron stars with luminosities < 1E34 erg/s, and hence thermal radiation remains a promising means to constraining neutron star radii.

arXiv comment14 pages, 9 figures, 5 tables, resubmitted to MNRAS after addressing referee's comments

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Cited by in corpus (11)

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• The gas-to-extinction ratio and the gas distribution in the Galaxy
• Neutron Star Mass-Radius Constraints of the Quiescent Low-mass X-ray Binaries X7 and X5 in the Globular Cluster 47 Tuc
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• Low-Mass X-ray Binaries
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• Constraining the properties of neutron star crusts with the transient low-mass X-ray binary Aql X-1
• The radius of the quiescent neutron star in the globular cluster M13
• The X-ray binary population in the Galactic Center revealed through multi-decade observations
• The Soft X-ray Spectrum of the High Mass X-Ray Binary V0332+53 in Quiescence
• Spectral analysis of the quiescent low-mass X-ray binary in the globular cluster M30