Akademik Veri Yönetim Sistemi
ASTROPHYSICAL JOURNAL LETTERS, cilt.908, sa.1, 2021 (SCI-Expanded)
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 similar or equal to 0.02 M-circle dot 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 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 (v) over dot = -2.1(7) x 10(-14) Hz s(-1) and to infer a pulsar surface dipole magnetic field strength of similar or equal to 10(9) G. We show that the mass transfer in the binary is likely nonconservative, and we discuss various scenarios for mass loss from the system.