4.7 Article

ASASSN-14ae: a tidal disruption event at 200 Mpc

Journal

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 445, Issue 3, Pages 3263-3277

Publisher

OXFORD UNIV PRESS
DOI: 10.1093/mnras/stu1922

Keywords

accretion, accretion discs; black hole physics; galaxies: nuclei

Funding

  1. NSF [AST-0908816, PHY-1101216, AST-9987045]
  2. Center for Cosmology and AstroParticle Physics at the Ohio State University
  3. Penn State the NASA Swift programme [NAS5-00136]
  4. NSF Telescope System Instrumentation Program (TSIP)
  5. Ohio Board of Regents
  6. Ohio State University Office of Research
  7. UK Science and Technology Facilities Council
  8. Robert Martin Ayers Sciences Fund
  9. Alfred P. Sloan Foundation
  10. National Science Foundation
  11. U.S. Department of Energy Office of Science
  12. University of Arizona
  13. Brazilian Participation Group
  14. Brookhaven National Laboratory
  15. Carnegie Mellon University
  16. University of Florida
  17. French Participation Group
  18. German Participation Group
  19. Harvard University
  20. Instituto de Astrofisica de Canarias
  21. Michigan State/Notre Dame/JINA Participation Group
  22. Johns Hopkins University
  23. Lawrence Berkeley National Laboratory
  24. Max Planck Institute for Astrophysics
  25. Max Planck Institute for Extraterrestrial Physics
  26. New Mexico State University
  27. New York University
  28. Ohio State University
  29. Pennsylvania State University
  30. University of Portsmouth
  31. Princeton University
  32. Spanish Participation Group
  33. University of Tokyo
  34. University of Utah
  35. Vanderbilt University
  36. University of Virginia
  37. University of Washington
  38. Yale University
  39. National Aeronautics and Space Administration
  40. Division Of Physics
  41. Direct For Mathematical & Physical Scien [1101216] Funding Source: National Science Foundation
  42. Science and Technology Facilities Council [ST/M000095/1, ST/M003035/1, ST/J001465/1] Funding Source: researchfish
  43. STFC [ST/M003035/1, ST/J001465/1, ST/M000095/1] Funding Source: UKRI

Ask authors/readers for more resources

ASASSN-14ae is a candidate tidal disruption event (TDE) found at the centre of SDSS J110840.11+340552.2 (d similar or equal to 200 Mpc) by the All-Sky Automated Survey for Supernovae (ASAS-SN). We present ground-based and Swift follow-up photometric and spectroscopic observations of the source, finding that the transient had a peak luminosity of L similar or equal to 8 x 10(43) erg s(-1) and a total integrated energy of E similar or equal to 1.7 x 10(50) erg radiated over the similar to 5 months of observations presented. The blackbody temperature of the transient remains roughly constant at T similar to 20 000 K while the luminosity declines by nearly 1.5 orders of magnitude during this time, a drop that is most consistent with an exponential, L proportional to e(-t/t0) with t(0) similar or equal to 39 d. The source has broad Balmer lines in emission at all epochs as well as a broad He II feature emerging in later epochs. We compare the colour and spectral evolution to both supernovae and normal AGN to show that ASASSN-14ae does not resemble either type of object and conclude that a TDE is the most likely explanation for our observations. At z = 0.0436, ASASSN-14ae is the lowest-redshift TDE candidate discovered at optical/UV wavelengths to date, and we estimate that ASAS-SN may discover 0.1-3 of these events every year in the future.

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