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Modeling accretion columns in accretion-powered pulsars

Context. Accretion-powered X-ray pulsars show complex spectral and timing behavior that reflects the extreme conditions near the neutron star. Modeling these observables remains challenging, particularly at high mass-accretion rates, Ṁ ≳ 1017 g s−1, where the extended accretion column plays a role i...

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Autori principali: Falkner S., Sokolova-Lapa E., Schwarm F.-W., Dauser T., Bissinger M., Ballhausen R., Falanga M., Ferrigno C., Postnov K. A., Schönherr G., Wolff M. T., Becker P. A., Pottschmidt K., Fürst F., Kretschmar P., Rothschild R. E., Hemphill P. B., Staubert R., Kreykenbohm I., Wilms J.
Natura: Artigo
Lingua:Inglês
Pubblicazione: EDP Sciences 2026-07-01
Serie:Astronomy & Astrophysics
Soggetti:
radiative transfer
relativistic processes
methods: numerical
stars: neutron
x-rays: binaries
Accesso online:https://www.aanda.org/articles/aa/full_html/2026/07/aa53642-24/aa53642-24.html
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