NICER observations of type-I X-ray bursts from the ultra-compact X-ray binary M15 X-2 - UTU Research Portal

A1 Refereed original research article in a scientific journal

NICER observations of type-I X-ray bursts from the ultra-compact X-ray binary M15 X-2

Authors: Díaz Teodori, Alejandra María; Kajava, Jari J. E.; Sánchez-Fernández, Celia; Sanna, Andrea; Ng, Mason; Poutanen, Juri

Publisher: EDP Sciences

Publishing place: LES ULIS CEDEX A

Publication year: 2025

Journal: Astronomy and Astrophysics

Journal name in source: Astronomy & Astrophysics

Journal acronym: ASTRON ASTROPHYS

Article number: A44

Volume: 695

Number of pages: 12

ISSN: 0004-6361

eISSN: 1432-0746

DOI: https://doi.org/10.1051/0004-6361/202452243

Web address : https://doi.org/10.1051/0004-6361/202452243

Self-archived copy’s web address: https://research.utu.fi/converis/portal/detail/Publication/491323667

Abstract

Type-I X-ray bursts are thermonuclear explosions caused by the unstable burning of accreted material on the surface of neutron stars. We report the detection of seven type-I X-ray bursts from the ultracompact X-ray binary M15 X-2 observed by the Neutron Star Interior Composition Explorer (NICER) during its 2022 outburst. We found all the bursts occurred in the soft state and exhibited similar light curve profiles, with no cases of photospheric radius expansion. Time-resolved spectroscopy showed clear deviations from the blackbody model during the first ten seconds of all the bursts. The fits were improved by using the enhanced persistent emission 'f(a)' method, which we interpret as evidence of burst-disk interaction. We compared the performance of these models against a neutron star atmosphere model and found it made no significant improvements. After analyzing the burst rise times and fuel composition, we propose that these bursts were powered by the burning of pure helium, confirming the ultracompact nature of the source.

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Funding information in the publication:
We thank the anonymous referee for their feedback that helped improve the manuscript. MADT acknowledges support from the EDUFI Fellowship and the Johannes Andersen Student Programme at the Nordic Optical Telescope. We acknowledge support from ESA through the ESA Space Science Faculty Visitor scheme (ESA-SCI-SC-LE-098 and ESA-SCI-SC-LE-203). M.N. is a Fonds de Recherche du Quebec – Nature et Technologies (FRQNT) postdoctoral fellow.