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Accretion in Stellar-Mass Black Holes at High X-ray Spectral Resolution

Published onMay 31, 2019
Accretion in Stellar-Mass Black Holes at High X-ray Spectral Resolution
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Abstract

Accretion disks around stellar-mass black holes are optimal regimes in which to make observational tests of seminal theory that applies across the mass scale. High X-ray spectral resolution will enable the most incisive tests. This white paper briefly reviews the key ideas and examines three case studies.

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