A comprehensive study of type I (thermonuclear) bursts in the new transient SRGA J144459.2604207
arXiv:2412.05779 · doi:10.3847/1538-4357/adadee
Abstract
We report an analysis of Insight-HXMT observations of the newly discovered accreting millisecond pulsar SRGA J144459.2604207. During the outburst, detected in 2024 February by SRG/ART-XC, the broadband persistent spectrum was well fitted by an absorbed Comptonization model. We detected 60 type I X-ray bursts in the Insight-HXMT medium energy (ME) data, and 37 were also detected with the low-energy (LE) telescope. By superimposing the Insight-HXMT/LE/ME/HE light curves of 37 bursts with similar profiles and intensities, we measured a deficit of X-rays in the keV energy band. By analyzing the time-resolved X-ray burst spectra, we determine the mean ratio of persistent to burst flux of . We estimate the average hydrogen mass fraction in the fuel at ignition, as , and constrain the burst fuel composition as . We found that 14 out of 60 X-ray bursts exhibited photospheric expansion, and thus we estimated the distance to the source as kpc. Combined with IXPE observations, the burst recurrence time increased from 1.55 to 8 hr as the local mass accretion rate decreased, which can be described as .
Published in ApJ
References in corpus (11)
- Thermonuclear (type-I) X-ray bursts observed by the Rossi X-ray Timing Explorer
- Evidence for enhanced persistent emission during sub-Eddington thermonuclear bursts
- X-Raying an Accretion Disk in Realtime: the Evolution of Ionized Reflection during a Superburst from 4U 1636-536
- Insight-HXMT observations of 4U~1636-536: Corona cooling revealed with single short type-I X-ray burst
- NICER observations of the evidence of Poynting-Robertson drag and disk reflection during type I X-ray bursts from 4U 1636536
- NICER views moderate, strong, and extreme photospheric expansion bursts from the ultracompact X-ray binary 4U 182030
- Type I X-ray bursts' spectra and fuel composition from the atoll and transient source 4U 173022
- SRG/ART-XC discovery of SRGAJ144459.2-604207: a well-tempered bursting accreting millisecond X-ray pulsar
- Similar phenomena at different scales: Black Holes, the Sun, Gamma-ray Bursts, Supernovae, Galaxies and Galaxy Clusters
- Robust inference of neutron-star parameters from thermonuclear burst observations
- Discovery of a long thermonuclear X-ray burst from the ultra-compact binary 4U 1850087
Cited by in corpus (5)
- Dense Matter in Neutron Stars with eXTP
- NinjaSat monitoring of Type-I X-ray bursts from the clocked burster SRGA J144459.2604207
- Quenching and recovery of persistent X-ray emission during a superburst in 4U 182030
- Timing and spectral studies of SRGA J144459.2604207 with NICER, Einstein Probe, IXPE, NuSTAR, Insight-HXMT and INTEGRAL during its 2024 outburst
- Long thermonuclear burst driven thermal-viscous instability of accretion disk: triggering an outburst-like X-ray flare