An upper observable black hole mass scale for tidal destruction events with thermal X-ray spectra
We comprehensively model the X-ray luminosity emergent from time-dependent relativistic accretion discs, developing analytical models of the X-ray luminosity of thermal disc systems as a function of black hole mass M, disc mass Md, and disc α-parameter. The X-ray properties of these solutions will b...
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| Médium: | Journal article |
| Jazyk: | English |
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Oxford University Press
2021
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