linkedin post 2021-07-28 16:37:50

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LOWER LIMIT. “An otherwise quiet MBH would show bright, beamed emission after the disruption of a WD. Therefore, detecting (or not detecting) signals from the tidal disruptions of WDs could place constraints on the MBH population.” (WD = white dwarf; MBH = Massive Black Hole). https://lnkd.in/djnsGi4 View in LinkedIn
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linkedin post 2021-07-28 16:34:28

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MASS DEPENDENT. “The possibility of detecting WD-TDEs is especially intriguing because the disruption of a WD is only visible if the mass of the BH, Mbh, is less than about 10(5) M⊙ or perhaps 10(6) M⊙ depending on the BH spin. For a more massive BH, the WD is ‘swallowed whole’ without disruption.” (WD = white dwarf; TDE = tidal disruption event). https://lnkd.in/djnsGi4 View in LinkedIn
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