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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主要な著者:	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
フォーマット:	Artigo
言語:	Inglês
出版事項:	IOP Publishing 2026-01-01
シリーズ:	The Astrophysical Journal
主題:	Stellar accretion disks Neutron stars Low-mass x-ray binary stars Spectropolarimetry Polarimetry
オンライン･アクセス:	https://doi.org/10.3847/1538-4357/ae5a8e
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