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X-Ray Polarization from the Atoll 4U 1735−44 Suggests a Low Inclination

X-ray polarimetry is a new tool capable of probing the geometry of accretion onto weakly magnetized neutron stars. Here we present the first X-ray spectropolarimetric results from coordinated observations of the atoll source 4U 1735−44, conducted with the Imaging X-ray Polarimetry Explorer (IXPE), N...

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Principais autores: María Alejandra Díaz Teodori, Anna Bobrikova, Andrea Gnarini, Francesco Ursini, Sofia V. Forsblom, Juri Poutanen, Alexander Salganik, Stefano Bianchi, Fiamma Capitanio, Massimo Cocchi, Sergio Fabiani, Ruben Farinelli, Philip Kaaret, Jari J. E. Kajava, Giorgio Matt, Mason Ng, Swati Ravi, Paolo Soffitta, Antonella Tarana, Silvia Zane
Format: Artigo
Sprog:Inglês
Udgivet: IOP Publishing 2026-01-01
Serier:The Astrophysical Journal
Fag:
Stellar accretion disks
Neutron stars
Low-mass x-ray binary stars
Spectropolarimetry
Polarimetry
Online adgang:https://doi.org/10.3847/1538-4357/ae5a8e
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