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...
मुख्य लेखकों: | Mummery, A, Balbus, SA |
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स्वरूप: | Journal article |
भाषा: | English |
प्रकाशित: |
Oxford University Press
2021
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समान संसाधन
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Hard X-ray emission from a Compton scattering corona in large black hole mass tidal disruption events
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A maximum X-ray luminosity scale of disc-dominated tidal destruction events
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The spectral evolution of disc dominated tidal disruption events
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The evolution of Kerr discs and late-time tidal disruption event light curves
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प्रकाशित: (2018) -
X-Ray Spectra of Black Hole X-Ray Binaries with Returning Radiation
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