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NGC 2403 XMM4: evidence for a super-Eddington neutron star with a possible transient pulsation

Luangtip, Wasutep; Roberts, Timothy P

NGC 2403 XMM4: evidence for a super-Eddington neutron star with a possible transient pulsation Thumbnail


Authors



Abstract

We present a study of the X-ray source NGC 2403 XMM4 (4XMM J073702.2+653934) based on 20 yr of archival observations
with XMM–Newton, Chandra, Swift, and NuSTAR. Although it has previously been classified as an ultraluminous X-ray source
(ULX), we show that itsluminosity rarely, if ever, passesthe 1039 erg s−1 threshold luminosity for a ULX. It does, however, behave
very similarly to ULXs, with its 0.3–10 keV spectra well described by two thermal components, the softer of which behaves
consistently with the expectations for an advection-dominated disc (L ∝ T1.49±0.85), and we find tentative evidence for an extra
spectral component above 10 keV. We also find moderately significant evidence for an absorption feature in one spectrum that
could originate in an outflowing wind, although a cyclotron resonance scattering feature is also a possibility. Most intriguingly,
we find a possible transient pulsation at ∼3.32 Hz in a short segment of one observation using an accelerated pulsation search.
This evidence suggests that NGC 2403 XMM4 is displaying many of the hallmarks of super-Eddington accretion at luminosities
in the range 5–10 × 1038 erg s−1 that, when considered alongside the putative pulsation, points to the presence of a neutron star
as the accreting object this system.

Citation

Luangtip, W., & Roberts, T. P. (2024). NGC 2403 XMM4: evidence for a super-Eddington neutron star with a possible transient pulsation. Monthly Notices of the Royal Astronomical Society, 528(1), 418-431. https://doi.org/10.1093/mnras/stae023

Journal Article Type Article
Acceptance Date Jan 3, 2024
Online Publication Date Jan 5, 2024
Publication Date 2024-02
Deposit Date May 22, 2024
Publicly Available Date May 22, 2024
Journal Monthly Notices of the Royal Astronomical Society
Print ISSN 0035-8711
Electronic ISSN 1365-2966
Publisher Royal Astronomical Society
Peer Reviewed Peer Reviewed
Volume 528
Issue 1
Pages 418-431
DOI https://doi.org/10.1093/mnras/stae023
Public URL https://durham-repository.worktribe.com/output/2456218

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Copyright Statement
© The Author(s) 2024.
Published by Oxford University Press on behalf of Royal Astronomical Society. This is an Open Access article distributed under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium,
provided the original work is properly cited





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