Polarization properties of the weakly magnetized neutron star X-ray binary GS 1826-238 in the high soft state
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Published version
Date
2023-02-01
Authors
Capitanio, Fiamma
Fabiani, Sergio
Gnarini, Andrea
Ursini, Francesco
Ferrigno, Carlo
Matt, Giorgio
Poutanen, Juri
Cocchi, Massimo
Mikusincova, Romana
Farinelli, Ruben
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Published version
Citation
F. Capitanio, S. Fabiani, A. Gnarini, F. Ursini, C. Ferrigno, G. Matt, J. Poutanen, M. Cocchi, R. Mikusincova, R. Farinelli, S. Bianchi, J.J.E. Kajava, F. Muleri, C. Sanchez-Fernandez, P. Soffitta, K. Wu, I. Agudo, L.A. Antonelli, M. Bachetti, L. Baldini, W.H. Baumgartner, R. Bellazzini, S.D. Bongiorno, R. Bonino, A. Brez, N. Bucciantini, S. Castellano, E. Cavazzuti, S. Ciprini, E. Costa, A.D. Rosa, E.D. Monte, L.D. Gesu, N.D. Lalla, A.D. Marco, I. Donnarumma, V. Doroshenko, M. Dovciak, S.R. Ehlert, T. Enoto, Y. Evangelista, R. Ferrazzoli, J.A. Garcia, S. Gunji, K. Hayashida, J. Heyl, W. Iwakiri, S.G. Jorstad, V. Karas, T. Kitaguchi, J.J. Kolodziejczak, H. Krawczynski, F.L. Monaca, L. Latronico, I. Liodakis, S. Maldera, A. Manfreda, F. Marin, A. Marinucci, A.P. Marscher, H.L. Marshall, I. Mitsuishi, T. Mizuno, C.-Y. Ng, S.L. O'Dell, N. Omodei, C. Oppedisano, A. Papitto, G.G. Pavlov, A.L. Peirson, M. Perri, M. Pesce-Rollins, P.-O. Petrucci, M. Pilia, A. Possenti, S. Puccetti, B.D. Ramsey, J. Rankin, A. Ratheesh, R.W. Romani, C. Sgrò, P. Slane, G. Spandre, T. Tamagawa, F. Tavecchio, R. Taverna, Y. Tawara, A.F. Tennant, N.E. Thomas, F. Tombesi, A. Trois, S.S. Tsygankov, R. Turolla, J. Vink, M.C. Weisskopf, F. Xie, S. Zane. 2023. "Polarization properties of the weakly magnetized neutron star X-ray binary GS 1826-238 in the high soft state" The Astrophysical Journal: an international review of astronomy and astronomical physics, Volume 943, Issue 2, pp.129-129. https://doi.org/10.3847/1538-4357/acae88
Abstract
The launch of the Imaging X-ray Polarimetry Explorer (IXPE) on 2021 December
9 has opened a new window in X-ray astronomy. We report here the results of the
first IXPE observation of a weakly magnetized neutron star, GS 1826-238,
performed on 2022 March 29-31 when the source was in a high soft state. An
upper limit (99.73% confidence level) of 1.3% for the linear polarization
degree is obtained over the IXPE 2-8 keV energy range. Coordinated INTEGRAL and
NICER observations were carried out simultaneously with IXPE. The spectral
parameters obtained from the fits to the broad-band spectrum were used as
inputs for Monte Carlo simulations considering different possible geometries of
the X-ray emitting region. Comparing the IXPE upper limit with these
simulations, we can put constraints on the geometry and inclination angle of GS
1826-238.
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© 2023. The Author(s). Published by the American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 license. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.