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Understanding High-Energy (UV and X-ray) Emission from AGB Stars—Episodic Accretion in Binary Systems
DOI: 10.3390/galaxies10030062 Bibcode: 2022Galax..10...62S

Sanz-Forcada, Jorge; Sahai, Raghvendra; Ortiz, Roberto +2 more

X-ray surveys of UV-emitting AGB stars show that ∼40% of objects with FUV emission and GALEX FUV/NUV flux ratio Rfuv/nuv ∼> 0.2 (fuvAGB stars) have variable X-ray emission characterized by very high temperatures (Tx∼35–160 MK) and luminosities (Lx∼0.002–0.2 L⊙), indicating the presence of accretion associated with a close binary companion. Howe…

2022 Galaxies
XMM-Newton 4
New Window on the Radio Emission from Galaxies, Clusters and Cosmic Web—Conference Summary
DOI: 10.3390/galaxies10010029 Bibcode: 2022Galax..10...29L

Venturi, Tiziana; Loi, Francesca

This manuscript summarizes the contributions presented and discussed during the conference "A new window on radio galaxies, clusters and cosmic web: current status and new challenges". The meeting was held online in March 2021. The works presented during the conference have been published in this associated Special Issue. Here, we outline the scie…

2022 Galaxies
XMM-Newton 0