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Tidal Disruptions of Binary Stars Ilya Mandel University of - PowerPoint PPT Presentation

Tidal Disruptions of Binary Stars Ilya Mandel University of Birmingham, UK (and Monash University, Melbourne) Collaborators: Yuri Levin (Monash), Ben Bradnick (Birmingham) Aspen, 2/11/2016 Tidal disruption [Rees, 1988; Gezari, 2014;


  1. Tidal Disruptions of Binary Stars Ilya Mandel University of Birmingham, UK (and Monash University, Melbourne) Collaborators: Yuri Levin (Monash), Ben Bradnick (Birmingham) Aspen, 2/11/2016

  2. Tidal disruption [Rees, 1988; Gezari, 2014; Guillochon & Ramirez-Ruiz, 2013 ]

  3. https://tde.space 3

  4. Tidal disruption [Rees, 1988; Gezari, 2014; Guillochon & Ramirez-Ruiz, 2013 ]

  5. Binary tidal disruptions [I. Mandel and Y. Levin. 2015. Double tidal disruptions in galactic nuclei. ApJ Letters, 805, L4. arXiv:1504.02787] 5

  6. Binary tidal disruptions 6

  7. Binary tidal disruptions 7

  8. Loss cone physics r full r min empty l *TD l LC L 8

  9. Double tidal disruptions 9

  10. Double tidal disruptions, I 10

  11. Double tidal disruptions, II 11

  12. Visualizations [ visualizations courtesy of James Guillochon] 12

  13. Simulations Mainetti et al., arXiv:1601.05478 13

  14. More unusual tidal disruptions? [Merloni et al., 2015, ArXiv: 1503.04870 Grupe et al., 2015, ArXiv: 1504.01389 ] 14

  15. Tidal disruption + jets [Bloom et al., 2011, Science, 333, 203; Levan et al., 2011, Science, 333, 199; also Burrows et al., 2011, Nature; Zauderer et al., 2011, Nature ] 15

  16. Tidal disruption + jets [Bloom et al., 2011, Science, 333, 203; Levan et al., 2011, Science, 333, 199; also Burrows et al., 2011, Nature; [Tchekhovskoy et al., 2014, MNRAS, 437, 2744: 
 Zauderer et al., 2011, Nature ] prompt jet requires magnetic flux > 10 29 G cm 2 ] 16

  17. What about the empty loss cone? Bradnick, Levin, Mandel, in prep. 17

  18. What about the empty loss cone? 18

  19. What about the empty loss cone? 19

  20. Conclusions § Around 5—10% of all TDEs are double TDEs of binaries » How important is the self-interaction of the tidal streams? » What would the spectrum look like? » Are these easy distinguish? § Tens of percent of binaries in the empty loss cone regime may merge before the merger product is tidally disrupted » What is the distinguishing observational signature? » Could the enhancement of the magnetic field due to recent merger power prompt jet formation? 20

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