QPO as the Rosetta Stone for understanding black hole accretion

DOI10.1002/ASNA.200510413zbMath1080.85006arXivastro-ph/0511382OpenAlexW3104918622WikidataQ68650781 ScholiaQ68650781MaRDI QIDQ5711701

Marek A. Abramowicz

Publication date: 8 December 2005

Published in: Astronomische Nachrichten (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/astro-ph/0511382

zbMATH Keywords

X-rays: quasi-periodic oscillations

Mathematics Subject Classification ID

Black holes (83C57) Quasi-periodic motions and invariant tori for nonlinear problems in mechanics (70K43) Galactic and stellar structure (85A15)

Related Items (1)

Difficulties of quantitative tests of the Kerr-hypothesis with X-ray observations of mass accreting black holes

Cites Work

• Oscillations of slender tori

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