XMMU J181227.8–181234: a new ultracompact X-ray binary candidate. Issue 3 (17th April 2019)

• Record Type: Journal Article
• Authors: Goodwin, A J; Galloway, D K; in 't Zand, J J M; Kuulkers, E; Bilous, A; Keek, L
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 486:Issue 3(2019)
• Page Start: 4149
• Page End: 4157
• Publication Date: 2019-04-17
• Subjects: stars: neutron -- X-rays: binaries -- X-rays: bursts; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/stz1094
• Languages: English
• ISSNs: 0035-8711

Abstract

ABSTRACT: We report the discovery of Type I (thermonuclear) X-ray bursts from the transient source XMMU J181227.8–181234 = XTE J1812–182. We found seven X-ray bursts in Rossi X-ray Timing Explorer observations during the 2008 outburst, confirming the source as a neutron star low-mass X-ray binary. Based on the measured burst fluence and the average recurrence time of 1.4$^{+0.9}_{-0.5}$ h, we deduce that the source is accreting almost pure helium ( X ≤ 0.1) fuel. Two bursts occurred just 18 min apart; the first short waiting time bursts observed in a source accreting hydrogen-poor fuel. Taking into consideration the effects on the burst and persistent flux due to the inferred system inclination of 30 ± 10°, we estimate the distance to be 14 ± 2 kpc, where we report the statistical uncertainty but note that there could be up to $20{{\ \rm per\ cent}}$ variation in the distance due to systematic effects discussed in the paper. The corresponding maximum accretion rate is 0.30 ± 0.05 times the Eddington limit. Based on the low hydrogen content of the accreted fuel and the short average recurrence time, we classify the source as a transient ultracompact low-mass X-ray binary.