SPECTRAL SOFTENING BETWEEN OUTBURST AND QUIESCENCE IN THE NEUTRON STAR LOW-MASS X-RAY BINARY SAX J1750.8-2900

• Main Authors: Allen, Jessamyn Leigh (Contributor), Linares, Manuel Alegret (Contributor), Homan, Jeroen (Contributor), Chakrabarty, Deepto (Contributor)
• Other Authors: Massachusetts Institute of Technology. Department of Physics (Contributor), MIT Kavli Institute for Astrophysics and Space Research (Contributor)
• Format: Article
• Language: English
• Published: Institute of Physics/American Astronomical Society, 2015-04-09T20:40:49Z.
• Subjects: Article
• Online Access: Get fulltext

 Tracking the spectral evolution of transiently accreting neutron stars between outburst and quiescence probes relatively poorly understood accretion regimes. Such studies are challenging because they require frequent monitoring of sources with luminosities below the thresholds of current all-sky X-ray monitors. We present the analysis of over 30 observations of the neutron star low-mass X-ray binary SAX J1750.8-2900 taken across four years with the X-ray telescope aboard Swift. We find spectral softening with decreasing luminosity both on long (~1 yr) and short (~days to week) timescales. As the luminosity decreases from 4 × 10[superscript 36] erg s[superscript −1] to $\sim 1\times {{10}^{35}}$ erg s[superscript −1] (0.5-10 keV), the power law photon index increases from 1.4 to 2.9. Although not statistically required, our spectral fits allow an additional soft component that displays a decreasing temperature as the luminosity decreases from 4 × 10[superscript 36] to 6 × 10[superscript 34] erg s[superscript −1]. Spectral softening exhibited by SAX J1750.8-2900 is consistent both with accretion emission whose spectral shape steepens with decreasing luminosity and also with being dominated by a changing soft component, possibly associated with accretion onto the neutron star surface, as the luminosity declines.