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Jim Fuller and Linhao Ma 2019 ApJL 881 L1

Models of angular momentum transport in massive evolving stars suggest that black holes born from single stars rotate very slowly (a < 0.01) regardless of the initial rotation rate.

A. R. Inglis et al 2019 ApJ 880 98

A systematic search for small-scale ephemeral coronal holes yielded only four examples over the time span of 2010–2015, with no corresponding signature seen in solar wind data at 1 AU.

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