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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Autors principals:	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.
Format:	Artigo
Idioma:	Inglês
Publicat:	EDP Sciences 2026-07-01
Col·lecció:	Astronomy & Astrophysics
Matèries:	radiative transfer relativistic processes methods: numerical stars: neutron x-rays: binaries
Accés en línia:	https://www.aanda.org/articles/aa/full_html/2026/07/aa53642-24/aa53642-24.html
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