Constraining the geometry of the dipping atoll 4U 1624–49 with X-ray spectroscopy and polarimetry

We present the spectro-polarimetric results obtained from simultaneous X-ray observations with IXPE, NuSTAR , and NICER of the dipping neutron star X-ray binary 4U 1624–49. This source is the most polarized Atoll source so far observed with IXPE, with a polarization degree of 2.7%±0.9% in the 2–8 keV band during the nondip phase and marginal evidence of an increasing trend with energy. The higher polarization degree compared to other Atolls can be explained by the high inclination of the system ( i ≈ 60°). The spectra are well described by the combination of soft thermal emission, a Comptonized component, and reflection of soft photons off the accretion disk. During the dips, the hydrogen column density of the highly ionized absorber increases while the ionization state decreases. The Comptonized radiation seems to be the dominant contribution to the polarized signal, with additional reflected photons that contribute significantly even though their fraction in the total flux is not high.

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Publication Details

Journal
Astronomy and Astrophysics
Published
2024-08-12
DOI
https://doi.org/10.1051/0004-6361/202450716
Citations
8
Primary Topic
Astrophysical Phenomena and Observations
Type
article
Field-Weighted Citation Impact
2.65

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article

Constraining the geometry of the dipping atoll 4U 1624–49 with X-ray spectroscopy and polarimetry

Juri Poutanen, F. Ursini, G. Matt, M. Lynne Saade et al.
8 citations
Astronomy and Astrophysics
Astrophysical Phenomena and Observations
2.65
article

Constraining the geometry of the dipping atoll 4U 1624–49 with X-ray spectroscopy and polarimetry

Juri Poutanen, F. Ursini, G. Matt, M. Lynne Saade, Fiamma Capitanio, Andrea Gnarini, P. Kaaret, S. Bianchi, Wenda Zhang
article en
8 citations

Abstract

We present the spectro-polarimetric results obtained from simultaneous X-ray observations with IXPE, NuSTAR , and NICER of the dipping neutron star X-ray binary 4U 1624–49. This source is the most polarized Atoll source so far observed with IXPE, with a polarization degree of 2.7%±0.9% in the 2–8 keV band during the nondip phase and marginal evidence of an increasing trend with energy. The higher polarization degree compared to other Atolls can be explained by the high inclination of the system ( i ≈ 60°). The spectra are well described by the combination of soft thermal emission, a Comptonized component, and reflection of soft photons off the accretion disk. During the dips, the hydrogen column density of the highly ionized absorber increases while the ionization state decreases. The Comptonized radiation seems to be the dominant contribution to the polarized signal, with additional reflected photons that contribute significantly even though their fraction in the total flux is not high.

Astronomy and AstrophysicsVol. 690
Roma Tre University (IT), Marshall Space Flight Center (US), Universities Space Research Association (US), University of Turku (FI), Chinese Academy of Sciences (CN), Institute for Space Astrophysics and Planetology (IT), National Astronomical Observatories (CN)
National Aeronautics and Space Administration, California Institute of Technology, National Natural Science Foundation of China, Chinese Academy of Sciences, Agenzia Spaziale Italiana, Istituto Nazionale di Astrofisica, Jet Propulsion Laboratory, Marshall Space Flight Center, Goddard Space Flight Center
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Openalex Percentile: Top 11%
Astrophysical Phenomena and Observations
2.65
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