Vertical wind structure in an X-ray binary revealed by a precessing accretion disk

Kosec P, Kara E, Fabian AC, Fuerst F, Pinto C, Psaradaki I, Reynolds CS, Rogantini D, Walton DJ, Ballhausen R, Canizares C, Dyda S, Staubert R, Wilms J (2023)

Publication Type: Journal article

Publication year: 2023

Journal

Nature Astronomy Nature Research

DOI: 10.1038/s41550-023-01929-7

Abstract

Kosec et al. analyse X-ray spectroscopic observations of outflowing hot material from an accreting neutron star. An innovative technique reveals the vertical distribution of the outflow structure, which is challenging to measure otherwise.

Authors with CRIS profile

Jörn Wilms Lehrstuhl für Astronomie und Astrophysik

Involved external institutions

Massachusetts Institute of Technology (MIT)

United States (USA) (US) University of Maryland

United States (USA) (US) European Space Astronomy Centre (ESAC)

Spain (ES) Institute of Space Astrophysics and Cosmic Physics / Palermo Istituto di Astrofisica Spaziale e Fisica Cosmica (IASF)

Italy (IT) University of Michigan

United States (USA) (US) University of Virginia (UVA)

United States (USA) (US) University of Hertfordshire

United Kingdom (GB) Eberhard Karls Universität Tübingen

Germany (DE)

How to cite

APA:

Kosec, P., Kara, E., Fabian, A.C., Fuerst, F., Pinto, C., Psaradaki, I.,... Wilms, J. (2023). Vertical wind structure in an X-ray binary revealed by a precessing accretion disk. Nature Astronomy. https://doi.org/10.1038/s41550-023-01929-7

MLA:

Kosec, P., et al. "Vertical wind structure in an X-ray binary revealed by a precessing accretion disk." Nature Astronomy (2023).

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