An inner disk below the ADAF: the intermediate spectral state of black hole accretion
B. F. Liu, F. Meyer, E. Meyer‐Hofmeister
Abstract
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B. F. Liu, F. Meyer, E. Meyer‐Hofmeister
Abstract
Open-access reader
Aims.The hard and soft spectral states of black hole accretion are understood as connected with ADAF accretion (truncated disk) and standard disk accretion, respectively. However, observations indicate the existence of cool gas in the inner region at times when the disk is already truncated outside. We try to shed light on these not yet understood intermediate states.
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Aims.The hard and soft spectral states of black hole accretion are understood as connected with ADAF accretion (truncated disk) and standard disk accretion, respectively. However, observations indicate the existence of cool gas in the inner region at times when the disk is already truncated outside. We try to shed light on these not yet understood intermediate states.
Key concepts: Accretion disc, Accretion (finance), Physics, Astrophysics, Intermediate polar, Thin disk, Astronomy, Stars