NICER Discovery of Millisecond X-ray Pulsations and an Ultracompact Orbit in IGR J17494-3030

TL;DR

This paper reports the discovery of millisecond X-ray pulsations and an ultracompact orbit in the low-mass X-ray binary IGR J17494-3030, revealing details about its pulsar spin, magnetic field, and mass transfer behavior.

Contribution

It presents the first detection of coherent X-ray pulsations in IGR J17494-3030 and characterizes its ultracompact binary nature and long-term pulsar spin-down rate.

Findings

Detected 376.05 Hz X-ray pulsations in 2020 NICER data.

Measured a long-term pulsar spin-down rate of -2.1×10⁻¹⁴ Hz/s.

Inferred a pulsar magnetic field strength of approximately 10⁹ G.

Abstract

We report the detection of 376.05 Hz (2.66 ms) coherent X-ray pulsations in NICER observations of a transient outburst of the low-mass X-ray binary IGR J17494-3030 in 2020 October/November. The system is an accreting millisecond X-ray pulsar in a 75 minute ultracompact binary. The mass donor is most likely a $\simeq 0.02 M_\odot$ finite-entropy white dwarf composed of He or C/O. The fractional rms pulsed amplitude is 7.4%, and the soft (1-3 keV) X-ray pulse profile contains a significant second harmonic. The pulsed amplitude and pulse phase lag (relative to our mean timing model) are energy-dependent, each having a local maximum at 4 keV and 1.5 keV, respectively. We also recovered the X-ray pulsations in archival 2012 XMM-Newton observations, allowing us to measure a long-term pulsar spin-down rate of $\dot\nu = -2.1(7)\times10^{-14}$ Hz/s and to infer a pulsar surface dipole magnetic field strength of $\simeq 10^9$ G. We show that the mass transfer in the binary is likely non-conservative, and we discuss various scenarios for mass loss from the system.