A catalogue of intermediate-duration Type I X-ray bursts observed with the INTEGRAL satellite. Issue 2 (28th March 2020)

• Record Type: Journal Article
• Authors: Alizai, K; Chenevez, J; Brandt, S; Lund, N
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 494:Issue 2(2020)
• Page Start: 2509
• Page End: 2522
• Publication Date: 2020-03-28
• Subjects: stars: neutron -- X-rays: binaries -- X-rays: bursts; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/staa831
• Languages: English
• ISSNs: 0035-8711

Abstract

ABSTRACT: We present a catalogue of long-duration bursts observed with the Joint European X-ray Monitor and IBIS/ISGRI instruments onboard the INTEGRAL satellite. The 14 bursts have e-folding times ranging from 55 s to ≈17 min, and are therefore classified as intermediate-duration bursts, caused by the ignition of an unusually thick helium layer. Though seven events have already been reported in literature, we have systematically reanalysed the whole sample. We find three new photospheric radius expansion bursts, which are not reported in the literature, allowing us to provide a new estimate of the distances to these sources. We apply the enhanced persistent emission method (also known as the f a method) on sources with detectable persistent emission prior to a burst, in order to follow the evolution of the accretion rate during the burst. Although we do not get significantly better fits, the evolution of the f a factor shows an indicative behaviour, which we discuss.