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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| Autores principales: | Luna, G.J.M., Mukai, K., Sokoloski, J.L., Lucy, A.B., Cusumano, G., Segreto, A., Jaque Arancibia, M., Nuñez, N.E., Puebla, R.E., Nelson, T., Walter, F. |
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| Formato: | JOUR |
| Materias: | |
| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_00046361_v616_n_p_Luna |
| Aporte de: |
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