A magnetar outburst with atypical evolution: the case of Swift J1555.2-5402

TL;DR

This study presents a detailed 29-month X-ray and radio monitoring of the magnetar Swift J1555.2-5402's atypical outburst, revealing unusual flux decay, a shrinking hot spot, and persistent high temperature, challenging existing models.

Contribution

It provides the first extensive multi-instrument observational analysis of this magnetar's unusual outburst evolution, highlighting features that question current theoretical frameworks.

Findings

Flux remained >1e-11 erg/cm^2/s for ~500 days

Spectrum dominated by a stable blackbody with shrinking radius

No radio bursts or periodic emission detected

Abstract

The magnetar Swift J1555.2-5402 was discovered in outburst on 2021 June 3 by the Burst Alert Telescope on board the Swift satellite. Early X-ray follow-up revealed a spin period P~3.86 s, a period derivative Pdot~3e-11 s/s, dozens of short bursts, and an unusually flux decline. We report here on the X-ray monitoring of Swift J1555.2-5402 over the first ~29 months of its outburst with Swift, NICER, NuSTAR, INTEGRAL and Insight-HXMT, as well as radio observations with Parkes soon after the outburst onset. The observed 0.3-10 keV flux remained at levels >~1e-11 erg/cm^2/s for nearly 500 days before dropping by a factor of ~10 from its June 2021 peak towards the end of the monitoring campaign. During this time span, the spectrum was dominated by a single blackbody, with temperature attaining approximately a constant value (~1.2 keV) while the inferred radius shrank from ~1.7 km to ~0.3 km (assuming a source distance of 10 kpc). The long-term spin-down rate (Pdot~3.6e-11 s/s) is only ~15 % higher than that measured in the first 30 days. No periodic or burst-like radio emission was detected, in line with what has been previously reported using different radio facilities. The persistently high temperature, shrinking hotspot, and a prolonged bright flux plateau followed by a fast dimming observed during the outburst evolution pose a challenge for the outburst mechanisms proposed so far.