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This paper summarises our current understanding of the spectral continuum components observed in black hole X‐ray binaries. The consequences for theoretical models are discussed with an emphasis on the constraints set by observations on the nature of the X‐ray corona in different spectral states. (© 2016 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)

Spectral components in black hole X‐ray binaries