Black Hole accretion under the X-ray microscope

0573519 - ASÚ 2024 RIV eng U - Uspořádání akce
Miniutti, G. - Schartel, N. - Bianchi, S. - Czerny, B. - De Marco, B. - Done, C. - Dovčiak, Michal … celkem 20 autorů
Black Hole accretion under the X-ray microscope.
[Madrid, 14.06.2022-17.06.2022, (W-WRD 150/147)]
Institucionální podpora: RVO:67985815
Klíčová slova: extreme variability events * active galactic nuclei * BH X-ray binaries
Obor OECD: Astronomy (including astrophysics,space science)

The meeting will focus on black hole accretion and its consequences, following the accretion flow from the direct relativistic environment of the black holes out to galactic scales. The two flagship X-ray missions XMM-Newton and Chandra are constantly expanding the frontiers of our knowledge. Many further international X-ray observatories, like NuSTAR, NICER, SRG / eROSITA & ART-XC, Swift, MAXI, Integral, HXMT and AstroSAT, are continuously discovering new phenomena. Multi-wavelength observations, complementing the X-ray data, are often crucial to sharpen our view of the accretion phenomenon and its effects on its surroundings. The meeting aims at providing an opportunity to discuss new results, open questions, and pathways for future progress in the field.
Trvalý link: https://hdl.handle.net/11104/0343952