A superburst candidate in EXO 1745--248 as a challenge to thermonuclear ignition models

TL;DR

This paper reports a likely superburst from the neutron star in EXO 1745-248, challenging existing thermonuclear ignition models due to its properties and the inferred ignition conditions.

Contribution

It presents the first detailed analysis of a superburst candidate in EXO 1745-248, highlighting discrepancies with current theoretical models.

Findings

The flare's decay time was 6-11 hours.

The radiated energy was estimated at 2-9 x 10^42 erg.

The ignition column depth is about 10^12 g cm^-2.

Abstract

We report on Chandra, RXTE, Swift/BAT and MAXI observations of a ~1 day X-ray flare and subsequent outburst of a transient X-ray source observed in October-November 2011 in the globular cluster Terzan 5. We show that the source is the same as the transient that was active in 2000, i.e., the neutron star low-mass X-ray binary EXO 1745-248. For the X-ray flare we estimate a 6-11 hr exponential decay time and a radiated energy of 2-9 x 10^42 erg. These properties, together with strong evidence of decreasing blackbody temperature during the flare decay, are fully consistent with what is expected for a thermonuclear superburst. We use the most recent superburst models and estimate an ignition column depth of ~10^12 g cm^-2 and an energy release between 0.1-2 x 10^18 erg g^-1, also consistent with expected superburst values. We conclude therefore that the flare was most probably a superburst. We discuss our results in the context of theoretical models and find that even when assuming a few days of low level accretion before the superburst onset (which is more than what is suggested by the data), the observations of this superburst are very challenging for current superburst ignition models.