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...
Principais autores: | Mummery, A, Balbus, SA |
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Formato: | Journal article |
Idioma: | English |
Publicado em: |
Oxford University Press
2021
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