Constraining the Accretion Geometry of the Intermediate Polar EX Hya Using NuSTAR, Swift, and Chandra Observations

In magnetically accreting white dwarfs, the height above the white dwarf surface where the standing shock is formed is intimately related with the accretion rate and the white dwarf mass. However, it is difficult to measure. We obtained new data with NuSTAR and Swift that, together with archival Cha...

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Detalles Bibliográficos
Publicado:	2018
Materias:	novae, cataclysmic variables radiation mechanisms: general X-rays: individual (EX Hydrae)
Acceso en línea:	https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_20418205_v852_n1_p_Luna http://hdl.handle.net/20.500.12110/paper_20418205_v852_n1_p_Luna
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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