_version_ 1866911319450451968
author Mikušincová, Romana
Marra, Lorenzo
Manikantan, Hemanth
Bianchi, Stefano
Capitanio, Fiamma
Chakraborty, Sudip
Ciancarella, Raul
Costa, Enrico
De Angelis, Nicolas
Del Santo, Melania
Fabiani, Sergio
Ferrazzoli, Riccardo
Gianolli, Vittoria E.
Gnarini, Andrea
Ingram, Adam
Mandel, Shifra
Mastroserio, Guglielmo
Matt, Giorgio
Mori, Kaya
Muleri, Fabio
Pagliarella, Simone
Parra, Maxime
Petrucci, P. O.
Podgorný, Jakub
Poutanen, Juri
Ravi, Swati
Soffitta, Paolo
Steiner, James F.
Tarana, Antonella
Taverna, Roberto
Ursini, Francesco
Veledina, Alexandra
Vincentelli, Federico M.
Yilmaz, Anastasiya
De Marco, Barbara
Gupta, Maitrayee
Loktev, Vladislav
Russell, Thomas D.
Svoboda, Jiří
Tombesi, Francesco
Zhang, Shuo
author_facet Mikušincová, Romana
Marra, Lorenzo
Manikantan, Hemanth
Bianchi, Stefano
Capitanio, Fiamma
Chakraborty, Sudip
Ciancarella, Raul
Costa, Enrico
De Angelis, Nicolas
Del Santo, Melania
Fabiani, Sergio
Ferrazzoli, Riccardo
Gianolli, Vittoria E.
Gnarini, Andrea
Ingram, Adam
Mandel, Shifra
Mastroserio, Guglielmo
Matt, Giorgio
Mori, Kaya
Muleri, Fabio
Pagliarella, Simone
Parra, Maxime
Petrucci, P. O.
Podgorný, Jakub
Poutanen, Juri
Ravi, Swati
Soffitta, Paolo
Steiner, James F.
Tarana, Antonella
Taverna, Roberto
Ursini, Francesco
Veledina, Alexandra
Vincentelli, Federico M.
Yilmaz, Anastasiya
De Marco, Barbara
Gupta, Maitrayee
Loktev, Vladislav
Russell, Thomas D.
Svoboda, Jiří
Tombesi, Francesco
Zhang, Shuo
contents 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 $ \sim $1.5' of the Galactic center, was observed serendipitously during a MAXI J1744-294 observation with a duration of 150 ks. The complex nature of the region in which AX J1745.6-2901 is located poses a challenge for studying its polarization. By performing a detailed analysis of the contamination from MAXI J1744-294 and the Galactic center diffuse emission, we find the source polarization degree PD = 14.7$\% \pm$ 4.0$\%$ and polarization angle PA = 122$^\circ \pm 8^\circ$. The phase-resolved analysis shows increase in polarization during the eclipse phase, with PD = 34.2$\% \pm$ 8.7$\%$, suggesting that the polarization-inducing mechanisms are of scattering nature, probably originating from disk winds.
format Preprint
id arxiv_https___arxiv_org_abs_2512_13182
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle The First X-Ray Polarimetry of an Eclipsing Low-Mass X-Ray Binary: Serendipitous IXPE Observation of AX J1745.6-2901
Mikušincová, Romana
Marra, Lorenzo
Manikantan, Hemanth
Bianchi, Stefano
Capitanio, Fiamma
Chakraborty, Sudip
Ciancarella, Raul
Costa, Enrico
De Angelis, Nicolas
Del Santo, Melania
Fabiani, Sergio
Ferrazzoli, Riccardo
Gianolli, Vittoria E.
Gnarini, Andrea
Ingram, Adam
Mandel, Shifra
Mastroserio, Guglielmo
Matt, Giorgio
Mori, Kaya
Muleri, Fabio
Pagliarella, Simone
Parra, Maxime
Petrucci, P. O.
Podgorný, Jakub
Poutanen, Juri
Ravi, Swati
Soffitta, Paolo
Steiner, James F.
Tarana, Antonella
Taverna, Roberto
Ursini, Francesco
Veledina, Alexandra
Vincentelli, Federico M.
Yilmaz, Anastasiya
De Marco, Barbara
Gupta, Maitrayee
Loktev, Vladislav
Russell, Thomas D.
Svoboda, Jiří
Tombesi, Francesco
Zhang, Shuo
High Energy Astrophysical Phenomena
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 $ \sim $1.5' of the Galactic center, was observed serendipitously during a MAXI J1744-294 observation with a duration of 150 ks. The complex nature of the region in which AX J1745.6-2901 is located poses a challenge for studying its polarization. By performing a detailed analysis of the contamination from MAXI J1744-294 and the Galactic center diffuse emission, we find the source polarization degree PD = 14.7$\% \pm$ 4.0$\%$ and polarization angle PA = 122$^\circ \pm 8^\circ$. The phase-resolved analysis shows increase in polarization during the eclipse phase, with PD = 34.2$\% \pm$ 8.7$\%$, suggesting that the polarization-inducing mechanisms are of scattering nature, probably originating from disk winds.
title The First X-Ray Polarimetry of an Eclipsing Low-Mass X-Ray Binary: Serendipitous IXPE Observation of AX J1745.6-2901
topic High Energy Astrophysical Phenomena
url https://arxiv.org/abs/2512.13182