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    Candidate Tidal Disruption Event AT2019fdr Coincident with a High-Energy Neutrino

    89851.pdf (1.253Mb)
    Access Status
    Open access
    Authors
    Reusch, S.
    Stein, R.
    Kowalski, M.
    Van Velzen, S.
    Franckowiak, A.
    Lunardini, C.
    Murase, K.
    Winter, W.
    Miller-Jones, James
    Kasliwal, M.M.
    Gilfanov, M.
    Garrappa, S.
    Paliya, V.S.
    Ahumada, T.
    Anand, S.
    Barbarino, C.
    Bellm, E.C.
    Brinnel, V.
    Buson, S.
    Cenko, S.B.
    Coughlin, M.W.
    De, K.
    Dekany, R.
    Frederick, S.
    Gal-Yam, A.
    Gezari, S.
    Giroletti, M.
    Graham, M.J.
    Karambelkar, V.
    Kimura, S.S.
    Kong, A.K.H.
    Kool, E.C.
    Laher, R.R.
    Medvedev, P.
    Necker, J.
    Nordin, J.
    Perley, D.A.
    Rigault, M.
    Rusholme, B.
    Schulze, S.
    Schweyer, T.
    Singer, L.P.
    Sollerman, J.
    Strotjohann, N.L.
    Sunyaev, R.
    Van Santen, J.
    Walters, R.
    Zhang, B.T.
    Zimmerman, E.
    Date
    2022
    Type
    Journal Article
    
    Metadata
    Show full item record
    Citation
    Reusch, S. and Stein, R. and Kowalski, M. and Van Velzen, S. and Franckowiak, A. and Lunardini, C. and Murase, K. et al. 2022. Candidate Tidal Disruption Event AT2019fdr Coincident with a High-Energy Neutrino. Physical Review Letters. 128 (22): ARTN 221101.
    Source Title
    Physical Review Letters
    DOI
    10.1103/PhysRevLett.128.221101
    ISSN
    0031-9007
    Faculty
    Faculty of Science and Engineering
    School
    School of Elec Eng, Comp and Math Sci (EECMS)
    Funding and Sponsorship
    http://purl.org/au-research/grants/arc/DP200102471
    Remarks

    Copyright © 2022 American Physical Society

    URI
    http://hdl.handle.net/20.500.11937/90027
    Collection
    • Curtin Research Publications
    Abstract

    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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