Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 445, Issue 3, Pages 3263-3277Publisher
OXFORD UNIV PRESS
DOI: 10.1093/mnras/stu1922
Keywords
accretion, accretion discs; black hole physics; galaxies: nuclei
Categories
Funding
- NSF [AST-0908816, PHY-1101216, AST-9987045]
- Center for Cosmology and AstroParticle Physics at the Ohio State University
- Penn State the NASA Swift programme [NAS5-00136]
- NSF Telescope System Instrumentation Program (TSIP)
- Ohio Board of Regents
- Ohio State University Office of Research
- UK Science and Technology Facilities Council
- Robert Martin Ayers Sciences Fund
- Alfred P. Sloan Foundation
- National Science Foundation
- U.S. Department of Energy Office of Science
- University of Arizona
- Brazilian Participation Group
- Brookhaven National Laboratory
- Carnegie Mellon University
- University of Florida
- French Participation Group
- German Participation Group
- Harvard University
- Instituto de Astrofisica de Canarias
- Michigan State/Notre Dame/JINA Participation Group
- Johns Hopkins University
- Lawrence Berkeley National Laboratory
- Max Planck Institute for Astrophysics
- Max Planck Institute for Extraterrestrial Physics
- New Mexico State University
- New York University
- Ohio State University
- Pennsylvania State University
- University of Portsmouth
- Princeton University
- Spanish Participation Group
- University of Tokyo
- University of Utah
- Vanderbilt University
- University of Virginia
- University of Washington
- Yale University
- National Aeronautics and Space Administration
- Division Of Physics
- Direct For Mathematical & Physical Scien [1101216] Funding Source: National Science Foundation
- Science and Technology Facilities Council [ST/M000095/1, ST/M003035/1, ST/J001465/1] Funding Source: researchfish
- 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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