X-ray, UV, and optical observations of the accretion disk and boundary layer in the symbiotic star RT Crucis

Compared to mass transfer in cataclysmic variables, the nature of accretion in symbiotic binaries in which red giants transfer material to white dwarfs (WDs) has been difficult to uncover. The accretion flows in a symbiotic binary are most clearly observable, however, when there is no quasi-steady s...

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Detalles Bibliográficos
Publicado:	2018
Materias:	Accretion, accretion disks Binaries: symbiotic X-rays: binaries Binary alloys Boundary layers Giant stars Mass transfer Photometry White dwarfs X rays Accretion , accretion disks Burst alert telescopes Cataclysmic variables Optical observations Reflection amplitude Ultraviolet optical telescopes X-rays: Binaries X ray detectors
Acceso en línea:	https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v616_n_p_Luna http://hdl.handle.net/20.500.12110/paper_00046361_v616_n_p_Luna
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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