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. 2017 Nov 29;20(1):7. doi: 10.1007/s41114-017-0008-x

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© The Author(s) 2017

Open AccessThis article is distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution, and reproduction in any medium, provided you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made.

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Fig. 30 — Cut of 3D rest-mass density profile (colored volume rendering) of a magnetized rotating, collapsing supermassive star with magnetic-field lines indicated by white curves. The top panel corresponds to the time near BH formation, the middle panel is during the development of the incipient jet, and the bottom panel shows the fully developed incipient jet. (Image reproduced with permission from Sun et al. 2017, copyright by APS)