Authors

Adam Ingram, Newcastle University
Niek Bollemeijer, Anton Pannekoek Instituut voor Sterrenkunde
Alexandra Veledina, Turun yliopisto
Michal Dovčiak, Academy of Sciences of the Czech Republic
Juri Poutanen, Turun yliopisto
Elise Egron, Osservatorio Astronomico di Cagliari
Thomas D. Russell, INAF Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo
Sergei A. Trushkin, Special Astrophysical Observatory, Russian Academy of Sciences
Michela Negro, Louisiana State University
Ajay Ratheesh, Istituto Nazionale Di Astrofisica, Rome
Fiamma Capitanio, Istituto Nazionale Di Astrofisica, Rome
Riley Connors, Villanova University
Joseph Neilsen, Villanova University
Alexander Kraus, Max Planck Institute for Radio Astronomy
Maria Noemi Iacolina, Agenzia Spaziale Italiana
Alberto Pellizzoni, Osservatorio Astronomico di Cagliari
Maura Pilia, Osservatorio Astronomico di Cagliari
Francesco Carotenuto, University of Oxford
Giorgio Matt, Università degli Studi Roma Tre
Guglielmo Mastroserio, Università degli Studi di Milano
Philip Kaaret, NASA Marshall Space Flight Center
Stefano Bianchi, Università degli Studi Roma Tre
Javier A. García, NASA Goddard Space Flight Center
Matteo Bachetti, Osservatorio Astronomico di Cagliari
Kinwah Wu, UCL Mullard Space Science Laboratory
Enrico Costa, Istituto Nazionale Di Astrofisica, Rome
Melissa Ewing, Newcastle University
Vadim Kravtsov, Turun yliopisto
Henric Krawczynski, McDonnell Center for the Space Sciences
Vladislav Loktev, Turun yliopisto
Andrea Marinucci, Agenzia Spaziale Italiana
Lorenzo Marra, Università degli Studi Roma Tre
Romana Mikušincová, Istituto Nazionale Di Astrofisica, Rome

Document Type

Article

Publication Date

6-1-2024

Abstract

We report on an observational campaign on the bright black hole (BH) X-ray binary Swift J1727.8-1613 centered around five observations by the Imaging X-ray Polarimetry Explorer. These observations track for the first time the evolution of the X-ray polarization of a BH X-ray binary across a hard to soft state transition. The 2-8 keV polarization degree decreased from ∼4% to ∼3% across the five observations, but the polarization angle remained oriented in the north-south direction throughout. Based on observations with the Australia Telescope Compact Array, we find that the intrinsic 7.25 GHz radio polarization aligns with the X-ray polarization. Assuming the radio polarization aligns with the jet direction (which can be tested in the future with higher-spatial-resolution images of the jet), our results imply that the X-ray corona is extended in the disk plane, rather than along the jet axis, for the entire hard intermediate state. This in turn implies that the long (≳10 ms) soft lags that we measure with the Neutron star Interior Composition ExploreR are dominated by processes other than pure light-crossing delays. Moreover, we find that the evolution of the soft lag amplitude with spectral state does not follow the trend seen for other sources, implying that Swift J1727.8-1613 is a member of a hitherto undersampled subpopulation.

Publication Source (Journal or Book title)

Astrophysical Journal

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