Constraining the properties of the thermonuclear burst oscillation source XTE J1814−338 through pulse profile modelling
ABSTRACT Pulse profile modelling (PPM) is a comprehensive relativistic ray-tracing technique employed to determine the properties of neutron stars. In this study, we apply this technique to the Type I X-ray burster and accretion-powered millisecond pulsar XTE J1814−338, extracting its fundamental properties using PPM of its thermonuclear burst oscillations. Using data from its 2003 outburst, and a single uniform temperature hotspot model, we infer XTE J1814−338 to be located at a distance of $7.2^{+0.3}_{-0.4}$ kpc, with a mass of $1.21^{+0.05}_{-0.05}$ M$_\odot$ and an equatorial radius of $7.0^{+0.4}_{-0.4}$ km. Our results also offer insight into the time evolution of the hotspot but point to some potential shortcomings of the single uniform temperature hotspot model. We explore the implications of this result, including what we can learn about thermonuclear burst oscillation mechanisms and the importance of modelling the accretion contribution to the emission during the burst.
Authors
- S. Vinciguerra (ORCID: https://orcid.org/0000-0003-3068-6974)
- Tuomo Salmi (ORCID: https://orcid.org/0000-0001-6356-125X)
- Yves Kini (ORCID: https://orcid.org/0000-0002-0428-8430)
- В. Ф. Сулейманов (ORCID: https://orcid.org/0000-0003-3733-7267)
- Anna L. Watts (ORCID: https://orcid.org/0000-0002-1009-2354)
- A. V. Bilous (ORCID: https://orcid.org/0000-0002-7177-6987)
- Slavko Bogdanov (ORCID: https://orcid.org/0000-0002-9870-2742)
- D. K. Galloway (ORCID: https://orcid.org/0000-0002-6558-5121)
- Johannes Büchner (ORCID: https://orcid.org/0000-0003-0426-6634)
- Guru Partap Khalsa
Institutions
- Max Planck Institute for Extraterrestrial Physics (DE)
- Astronomical Institute of the Slovak Academy of Sciences (SK)
- Monash University (AU)
- Columbia University (US)
- University of Tübingen (DE)
- University of Amsterdam (NL)
- Netherlands Institute for Radio Astronomy (NL)
Publication Details
- Journal
- Monthly Notices of the Royal Astronomical Society
- Published
- 2024-10-21
- DOI
- https://doi.org/10.1093/mnras/stae2398
- Citations
- 29
- Primary Topic
- Gamma-ray bursts and supernovae
- Type
- article
- Field-Weighted Citation Impact
- 9.61
Funders
- National Aeronautics and Space Administration
- California Department of Fish and Game
- Deutsche Forschungsgemeinschaft
- Nuclear Safety and Security Commission
- H2020 European Research Council