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Roman Krivonos (Space Research Institute (IKI), Moscow, Russia)16/06/2026, 16:40
In my talk I will review our recent results related to the X-ray emission from the Galactic Center region, especially, the non-thermal emission of the Arches stellar cluster as observed with XMM-Newton and Chandra.
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Valentin Nezabudkin (Space Research Institute, MIPT)16/06/2026, 17:10
Recent studies based on XMM-Newton and SRG/ART-XC observations have reported an excess of X-ray emission per unit stellar mass in the Nuclear Stellar Disk (NSD) compared to regions farther from the Galactic Center. These results are based on hard X-ray measurements (4-12 keV) and studies of the Fe XXV emission line at 6.7 keV. In this work, we investigate the population of faint X-ray...
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