Authors

J. Podgorný, Academy of Sciences of the Czech Republic
J. Svoboda, Academy of Sciences of the Czech Republic
M. Dovčiak, Academy of Sciences of the Czech Republic
A. Veledina, Turun yliopisto
J. Poutanen, Turun yliopisto
P. Kaaret, NASA Marshall Space Flight Center
S. Bianchi, Università degli Studi Roma Tre
A. Ingram, Newcastle University
F. Capitanio, Istituto Nazionale Di Astrofisica, Rome
S. R. Datta, Academy of Sciences of the Czech Republic
E. Egron, Osservatorio Astronomico di Cagliari
H. Krawczynski, McDonnell Center for the Space Sciences
G. Matt, Università degli Studi Roma Tre
F. Muleri, Istituto Nazionale Di Astrofisica, Rome
P. O. Petrucci, Institut de Planétologie et d’Astrophysique de Grenoble (IPAG)
T. D. Russell, INAF Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo
J. F. Steiner, Harvard-Smithsonian Center for Astrophysics
N. Bollemeijer, Anton Pannekoek Instituut voor Sterrenkunde
M. Brigitte, Academy of Sciences of the Czech Republic
N. Castro Segura, Faculty of Science, Engineering and Medicine
R. Emami, Harvard-Smithsonian Center for Astrophysics
J. A. García, NASA Goddard Space Flight Center
K. Hu, McDonnell Center for the Space Sciences
M. N. Iacolina, Agenzia Spaziale Italiana
V. Kravtsov, Turun yliopisto
L. Marra, Università degli Studi Roma Tre
G. Mastroserio, Università degli Studi di Milano
T. Muñoz-Darias, Instituto Astrofisico de Canarias
E. Nathan, California Institute of Technology
M. Negro, Louisiana State University
A. Ratheesh, Istituto Nazionale Di Astrofisica, Rome
N. Rodriguez Cavero, McDonnell Center for the Space Sciences
R. Taverna, Università degli Studi di Padova

Document Type

Article

Publication Date

6-1-2024

Abstract

We report on the detection of X-ray polarisation in the black-hole X-ray binary Swift J1727.8-1613 during its dim hard spectral state by the Imaging X-ray Polarimetry Explorer (IXPE). This is the first detection of X-ray polarisation at the transition from the soft to the hard state in an X-ray binary. We find an averaged 2- 8 keV polarisation degree of (3.3 ± 0.4)% and a corresponding polarisation angle of 3 ±4, which matches the polarisation detected during the rising stage of the outburst, in September- October 2023, within 1σuncertainty. The observational campaign complements previous studies of this source and enables comparison of the X-ray polarisation properties of a single transient across the X-ray hardness-intensity diagram. The complete recovery of the X-ray polarisation properties, including the energy dependence, came after a dramatic drop in the X-ray polarisation during the soft state. The new IXPE observations in the dim hard state at the reverse transition indicate that the accretion properties, including the geometry of the corona, appear to be strikingly similar to the bright hard state during the outburst rise despite the X-ray luminosities differing by two orders of magnitude.

Publication Source (Journal or Book title)

Astronomy and Astrophysics

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