Candidate Tidal Disruption Event AT2019fdr Coincident with a High-Energy Neutrino Article Swipe
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Simeon Reusch
,
Robert Stein
,
M. Kowalski
,
Sjoert van Velzen
,
A. Franckowiak
,
Cecilia Lunardini
,
Kohta Murase
,
Walter Winter
,
J. C. A. Miller‐Jones
,
M. M. Kasliwal
,
M. Gilfanov
,
S. Garrappa
,
Vaidehi S. Paliya
,
Tomás Ahumada
,
Shreya Anand
,
C. Barbarino
,
Eric C. Bellm
,
V. Brinnel
,
S. Buson
,
S. B. Cenko
,
M. W. Coughlin
,
Kishalay De
,
Richard Dekany
,
Sara Frederick
,
A. Gal‐Yam
,
Suvi Gezari
,
M. Giroletti
,
M. J. Graham
,
Viraj Karambelkar
,
Shigeo S. Kimura
,
A. K. H. Kong
,
Erik C. Kool
,
Russ R. Laher
,
,
Jannis Necker
,
J. Nordin
,
D. A. Perley
,
M. Rigault
,
B. Rusholme
,
S. Schulze
,
T. Schweyer
,
L. P. Singer
,
J. Sollerman
,
N. L. Strotjohann
,
R. Sunyaev
,
J. V. Santen
,
Richard Walters
,
B. Theodore Zhang
,
E. Zimmerman
·
YOU?
·
· 2022
· Open Access
·
· DOI: https://doi.org/10.1103/physrevlett.128.221101
· OA: W3213617664
YOU?
·
· 2022
· Open Access
·
· DOI: https://doi.org/10.1103/physrevlett.128.221101
· OA: W3213617664
The origins of the high-energy cosmic neutrino flux remain largely unknown. Recently, one high-energy neutrino was associated with a tidal disruption event (TDE). Here we present AT2019fdr, an exceptionally luminous TDE candidate, coincident with another high-energy neutrino. Our observations, including a bright dust echo and soft late-time x-ray emission, further support a TDE origin of this flare. The probability of finding two such bright events by chance is just 0.034%. We evaluate several models for neutrino production and show that AT2019fdr is capable of producing the observed high-energy neutrino, reinforcing the case for TDEs as neutrino sources.
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