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Abstract Accretion onto black holes powers some of the most energetic sources in the Universe, yet its behaviour across the luminosity range remains poorly understood. Specifically, as the luminosity approaches the Eddington limit (LEdd), the inner accretion disk is expected to depart from the standard thin-disk solution, becoming vertically extended. The luminosity threshold and observational signatures of this transition remain, however, uncertain.
Supporting Information Filename Description uog29247-sup-0001-AppendixS1.docxWord 2007 document , 27 KB Appendix S1 Sample size estimation and multivariate distribution model for estimation of risk of pre-eclampsia (PE) uog29247-sup-0002-TableS1.docxWord 2007 document , 29.1 KB Table S1 Correlations between maternal cardiovascular biomarkers and echocardiographic measures evaluated in study population REFERENCES 1, , , et al.
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