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Observations of the Stellar Mass Black Hole Cygnus X-1 with the Imaging X-ray Polarimetry Explorer




AuthorsRodriguez Cavero Nicole, Krawczynski Henric, Muleri Fabio, Dovčiak Michal, Veledina Alexandra, Svoboda Jiri, Ingram Adam, Matt Giorgio, Garcia Javier, Loktev Vladislav, Negro Michela, Poutanen Juri, Kitaguchi Takao, Podgorny Jakub, Rankin John, Zhang Wenda; Cygnus X-1 Topical Working Group

PublisherAmerican Institute of Physics

Publication year2023

JournalBulletin of the American Astronomical Society

Book title HEAD20 Abstracts : The 20th Meeting of the High Energy Astrophysics Division

Volume55

Issue4

ISSN0002-7537

Web address https://baas.aas.org/pub/2023n4i109p06/release/1

Self-archived copy’s web addresshttps://research.utu.fi/converis/portal/detail/Publication/387034398


Abstract

X-ray polarization observations allow us to test accretion disk, corona, and emission models of stellar mass black holes in X-ray binaries. The Imaging X-ray Polarimetry Explorer (IXPE), launched on December 9, 2021, enables X-ray polarimetric observations with unprecedented sensitivity in the 2—8 keV energy range. We report here on the first IXPE observation of the black hole Cygnus X-1. We accompanied the May 2022 campaign with simultaneous Nuclear Spectroscopic Telescope Array (NuSTAR), Neutron Star Interior Composition Explorer (NICER), and INTErnational Gamma-Ray Astrophysics Laboratory (INTEGRAL) coverage to decompose the IXPE energy spectra into thermal disk, coronal, and reflection components. Furthermore, we present the implications of the polarization signature of Cygnus X-1 on the radio jet, the coronal geometry, and the inner accretion flow orientation.


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Last updated on 2024-26-11 at 17:05