Chandra/LETGS Studies of the Collisional Plasma in 4U 1626-67

Abstract

We present an analysis of \chandra/LETGS observations of the ultracompact X-ray binary (UCXB) 4U 1626$-$67, continuing our project to analyze the existing Chandra gratings data of this interesting source. The extremely low mass, hydrogen-depleted donor star provides a unique opportunity to study the properties and structure of the metal-rich accreted plasma. There are strong, double-peaked emission features of OVII-VIII and Ne IX-X, but no other identified emission lines are detected. Our spectral fit simultaneously models the emission line profiles and the plasma parameters, using a two-temperature collisionally-ionized plasma. Based on our line profile fitting, we constrain the inclination of the system to 25--60${}^{\circ }$ and the inner disk radius to $\sim$1500 gravitational radii, in turn constraining the donor mass to $\lesssim$0.026 M_sun, while our plasma modeling confirms previous reports of high neon abundance in the source, establishing a Ne/O ratio in the system of $0.47\pm 0.04$, while simultaneously estimating a very low Fe/O ratio of $0.0042\pm 0.0008$ and limiting the Mg/O ratio to less than 1% by number. We discuss these results in light of previous work.

accepted by the Astrophysical Main Journal, 16 pages, 13 figures

References in corpus (7)

• Thermal and Bulk Comptonization in Accretion-Powered X-Ray Pulsars
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Cited by in corpus (1)

• On the torque reversals of 4U 1626--67