SU Lyn: Diagnosing the Boundary Layer with UV and Hard X-Ray Data
Symbiotic stars in which the symbiotic phenomenon is powered solely by accretion, often at an average rate that is higher than in cataclysmic variable stars, provide an important opportunity to diagnose boundary layers around disk-Accreting white dwarfs. Here, we investigate SU Lyncis (SU Lyn), a re...
Guardado en:
Autores principales: | Lopes De Oliveira, R., Sokoloski, J.L., Luna, G.J.M., Mukai, K., Nelson, T. |
---|---|
Formato: | JOUR |
Materias: | |
Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_0004637X_v864_n1_p_LopesDeOliveira |
Aporte de: |
Ejemplares similares
-
SU Lyn: Diagnosing the Boundary Layer with UV and Hard X-Ray Data
Publicado: (2018) -
SU Lyncis, a hard X-ray bright M giant: Clues point to a large hidden population of symbiotic stars
por: Mukai, K., et al. -
X-ray, UV, and optical observations of the accretion disk and boundary layer in the symbiotic star RT Crucis
por: Luna, G.J.M., et al. -
SU Lyncis, a hard X-ray bright M giant: Clues point to a large hidden population of symbiotic stars
Publicado: (2016) -
Symbiotic stars in X-rays. II. Faint sources detected with XMM-Newton and Chandra
por: Nuñez, N.E., et al.