Evolution of relativistic thin discs with a finite ISCO stress: I. Stalled accretion
We present solutions to the relativistic thin disc evolutionary equation using an α-model for the turbulent stress tensor. Solutions with a finite stress at the innermost stable circular orbit (ISCO) give rise to bolometric light curves with a shallow power-law time dependence, in good agreement wit...
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| Format: | Journal article |
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Oxford University Press
2019
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