The First X-Ray Polarimetry of an Eclipsing Low-mass X-Ray Binary: Serendipitous IXPE Observation of AX J1745.6–2901

Abstract We present the first X-ray polarimetric measurement of the neutron star low-mass X-ray binary system AX J1745.6−2901 conducted by the Imaging X-ray Polarimetry Explorer (IXPE) satellite. This transient source, located within ∼1 <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:mover accent="true"> <mml:mrow> <mml:mi>.</mml:mi> </mml:mrow> <mml:mrow> <mml:mi>′</mml:mi> </mml:mrow> </mml:mover> </mml:math> 5 of the Galactic center, was observed serendipitously during a MAXI J1744−294 observation with a duration of 150 ks. The complex nature of the region in which AX J1745.6−2901 is located poses a challenge for studying its polarization. By performing a detailed analysis of the contamination from MAXI J1744−294 and the Galactic center diffuse emission, we find the source polarization degree PD = 14.7% ± 4.0% and polarization angle PA = 122° ± 8°. The phase-resolved analysis shows increase in polarization during the eclipse phase, with PD = 34.2% ± 8.7%, suggesting that the polarization-inducing mechanisms are of scattering nature, probably originating from disk winds.

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Journal
The Astrophysical Journal
Published
2026-06-30
DOI
https://doi.org/10.3847/1538-4357/ae7341
Primary Topic
Astrophysical Phenomena and Observations
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article
Field-Weighted Citation Impact
0.00

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article

The First X-Ray Polarimetry of an Eclipsing Low-mass X-Ray Binary: Serendipitous IXPE Observation of AX J1745.6–2901

F. Vincentelli, Jiří Svoboda, Juri Poutanen, F. Ursini et al.
The Astrophysical Journal
Astrophysical Phenomena and Observations
article

The First X-Ray Polarimetry of an Eclipsing Low-mass X-Ray Binary: Serendipitous IXPE Observation of AX J1745.6–2901

F. Vincentelli, Jiří Svoboda, Juri Poutanen, F. Ursini, G. Matt, Pierre-Olivier Petrucci, Adam Ingram, Raul Ciancarella, Kaya Mori, Lorenzo Marra, Francesco Tombesi, Fiamma Capitanio, Sudip Chakraborty, Maxime Parra, A. Tarana, Andrea Gnarini, Jakub Podgorný, Riccardo Ferrazzoli, Fabio Muleri, Romana Mikušincová, Hemanth Manikantan, Anastasiya Yilmaz, Shuo Zhang, Barbara De Marco, V. E. Gianolli, Guglielmo Mastroserio, Nicolas De Angelis, Vladislav Loktev, James F. Steiner, Shifra Mandel, Alexandra Veledina, S. Bianchi, Swati Ravi, Maitrayee Gupta, M. Del Santo, Sergio Fabiani, Paolo Soffitta, Enrico Costa, Simone Pagliarella, Roberto Taverna
article en

Abstract

Abstract We present the first X-ray polarimetric measurement of the neutron star low-mass X-ray binary system AX J1745.6−2901 conducted by the Imaging X-ray Polarimetry Explorer (IXPE) satellite. This transient source, located within ∼1 <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:mover accent="true"> <mml:mrow> <mml:mi>.</mml:mi> </mml:mrow> <mml:mrow> <mml:mi>′</mml:mi> </mml:mrow> </mml:mover> </mml:math> 5 of the Galactic center, was observed serendipitously during a MAXI J1744−294 observation with a duration of 150 ks. The complex nature of the region in which AX J1745.6−2901 is located poses a challenge for studying its polarization. By performing a detailed analysis of the contamination from MAXI J1744−294 and the Galactic center diffuse emission, we find the source polarization degree PD = 14.7% ± 4.0% and polarization angle PA = 122° ± 8°. The phase-resolved analysis shows increase in polarization during the eclipse phase, with PD = 34.2% ± 8.7%, suggesting that the polarization-inducing mechanisms are of scattering nature, probably originating from disk winds.

The Astrophysical JournalVol. 1005(1)
University of Rome Tor Vergata (IT), Roma Tre University (IT), Marshall Space Flight Center (US), Universities Space Research Association (US), University of Padua (IT), University of Turku (FI), Astronomical Observatory of Rome (IT), Czech Academy of Sciences, Astronomical Institute (CZ), Istituto Universitario di Studi Superiori di Pavia (IT), Brera Astronomical Observatory (IT), Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna (IT), Institute for Space Astrophysics and Planetology (IT), Istituto di Astrofisica Spaziale e Fisica Cosmica di Milano (IT), Istituto Nazionale di Fisica Nucleare, Roma Tor Vergata (IT), Center for Astrophysics Harvard & Smithsonian (US), University of Southampton (GB), Ehime University (JP), Institut des langues et cultures d'Europe, Amérique, Afrique, Asie et Australie (FR), Massachusetts Institute of Technology (US), Columbia University (US), Clemson University (US), Newcastle University (GB), Sapienza University of Rome (IT), KTH Royal Institute of Technology (SE), Michigan State University (US), National Institute for Astrophysics (IT), Université Grenoble Alpes (FR), Universitat Politècnica de Catalunya (ES)
National Aeronautics and Space Administration, Agenzia Spaziale Italiana, Istituto Nazionale di Astrofisica, Istituto Nazionale di Fisica Nucleare, Marshall Space Flight Center, Goddard Space Flight Center
Openalex Percentile: Top 98%
Astrophysical Phenomena and Observations
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