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Hydrodynamical simulation of the structure of the X-ray pulsar accretion channel: accounting for resonant scattering

Fuente: arXiv

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Detalles Bibliográficos
Autores principales:	Markozov, I. D., Kaminker, A. D., Potekhin, A. Y.
Formato:	Preprint
Publicado:	2023
Materias:	High Energy Astrophysical Phenomena
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

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