NICER observations of thermonuclear bursts from 4U 1728-34: Detection of oscillations prior to the onset of two bursts

TL;DR

This study analyzes NICER observations of 11 thermonuclear bursts from 4U 1728-34, revealing pre-burst oscillations and providing insights into burst timing and spectral properties, with implications for neutron star physics.

Contribution

First detection of burst oscillations prior to burst onset in 4U 1728-34, expanding understanding of burst oscillation behavior and neutron star surface phenomena.

Findings

Detected 11 X-ray bursts with NICER.

Found burst oscillations at 363 Hz during bursts.

Reported oscillations at 356 and 359 Hz before bursts.

Abstract

We present temporal and time-resolved spectral analyses of all the thermonuclear X-ray bursts observed from the neutron star low-mass X-ray binary (LMXB) 4U 1728-34 with NICER from June 2017 to September 2019. In total, we detected 11 X-ray bursts from the source and performed time-resolved spectroscopy. Unlike some of the earlier results for other bursting sources from NICER, our spectral results indicate that the use of a scaling factor for the persistent emission is not statistically necessary. This is primarily a result of the strong interstellar absorption in the line of sight towards 4U 1728-34, which causes the count rates to be significantly lower at low energies. We also searched for burst oscillations and detected modulations in six different bursts at around the previously known burst oscillation frequency of 363 Hz. Finally, we report the detection of oscillations prior to two bursts at 356 and 359 Hz, respectively. This is the first time in the literature where burst oscillations are detected before the rapid rise in X-ray flux, from any known burster. These oscillations disappear as soon as the burst rise starts and occur at a somewhat lower frequency than the oscillations we detect during the bursts.