λEdd . | Γ . | λ . | ηjet . | M *, max . |
---|---|---|---|---|
[1] . | [2] . | [3] . | [4] . | [5] . |
1.0 | 10 | −0.4 | 0.1 | 1.0 |
λEdd . | Γ . | λ . | ηjet . | M *, max . |
---|---|---|---|---|
[1] . | [2] . | [3] . | [4] . | [5] . |
1.0 | 10 | −0.4 | 0.1 | 1.0 |
*Col. [1]: Eddington ratio. Col. [2]: the Lorentz factor. Col. [3]: index for the MBH dependence of the TDE rate. Col. [4]: fraction of the intrinsic luminosity of the jet in LX. Col. [5]: upper mass boundary of disrupted stars in units of solar mass.
λEdd . | Γ . | λ . | ηjet . | M *, max . |
---|---|---|---|---|
[1] . | [2] . | [3] . | [4] . | [5] . |
1.0 | 10 | −0.4 | 0.1 | 1.0 |
λEdd . | Γ . | λ . | ηjet . | M *, max . |
---|---|---|---|---|
[1] . | [2] . | [3] . | [4] . | [5] . |
1.0 | 10 | −0.4 | 0.1 | 1.0 |
*Col. [1]: Eddington ratio. Col. [2]: the Lorentz factor. Col. [3]: index for the MBH dependence of the TDE rate. Col. [4]: fraction of the intrinsic luminosity of the jet in LX. Col. [5]: upper mass boundary of disrupted stars in units of solar mass.
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