15–19 Sept 2025
Cefalù (Palermo)
Europe/Rome timezone

X-ray Polarimetry of Neutron Star Low-Mass X-ray Binaries throughout the Z-track with IXPE

Not scheduled
15m
Palazzo Municipale - Sala delle Capriate (Cefalù (Palermo))

Palazzo Municipale - Sala delle Capriate

Cefalù (Palermo)

Cefalù (Palermo)

Speaker

Andrea Gnarini (Università degli Studi Roma Tre)

Description

Accreting, weakly magnetized Neutron Stars in Low-mass X-ray binaries (NS-LMXBs) are a fundamental laboratory to study radiation processes in the strong gravity regime. Z-sources are NS-LMXBs characterized by a wide Z-like three branches track in the Color-Color Diagram, typically accreting close to the Eddington limit.

In this talk, we discuss the spectro-polarimetric results obtained by IXPE (most often in coordination with other facilities) on NS-LMXBs in Z-state. Most of the known Z-sources were observed by IXPE during its two-year baseline phase, being the most polarized NS-LMXBs in the full 2-8 keV band and with a strong correlation between the observed polarization and the position along the Z-track. We will also provide an in-depth interpretation of these results, including also numerical simulations.

Affiliation Università degli Studi Roma Tre
E-mail andrea.gnarini@uniroma3.it

Author

Andrea Gnarini (Università degli Studi Roma Tre)

Co-authors

Prof. Stefano Bianchi (Università degli Studi Roma Tre) Dr Fiamma Capitanio (INAF-IAPS) Dr Massimo Cocchi (INAF-OAC) Dr Sergio Fabiani (INAF-IAPS) Dr Ruben Farinelli (INAF-OAS) Prof. Giorgio Matt (Università degli Studi Roma Tre) Dr Antonella Tarana (INAF-IAPS) Dr Francesco Ursini (Università degli Studi Roma Tre)

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