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    Illuminating gravitational waves: A concordant picture of photons from a neutron star merger

    Access Status
    Fulltext not available
    Authors
    Kasliwal, M.
    Nakar, E.
    Singer, L.
    Kaplan, D.
    Cook, D.
    Van Sistine, A.
    Lau, R.
    Fremling, C.
    Gottlieb, O.
    Jencson, J.
    Adams, S.
    Feindt, U.
    Hotokezaka, K.
    Ghosh, S.
    Perley, D.
    Yu, P.
    Piran, T.
    Allison, J.
    Anupama, G.
    Balasubramanian, A.
    Bannister, K.
    Bally, J.
    Barnes, J.
    Barway, S.
    Bellm, E.
    Bhalerao, V.
    Bhattacharya, D.
    Blagorodnova, N.
    Bloom, J.
    Brady, P.
    Cannella, C.
    Chatterjee, D.
    Cenko, S.
    Cobb, B.
    Copperwheat, C.
    Corsi, A.
    De, K.
    Dobie, D.
    Emery, S.
    Evans, P.
    Fox, O.
    Frail, D.
    Frohmaier, C.
    Goobar, A.
    Hallinan, G.
    Harrison, F.
    Helou, G.
    Hinderer, T.
    Ho, A.
    Horesh, A.
    Ip, W.
    Itoh, R.
    Kasen, D.
    Kim, H.
    Kuin, N.
    Kupfer, T.
    Lynch, Christene
    Madsen, K.
    Mazzali, P.
    Miller, A.
    Mooley, K.
    Murphy, T.
    Ngeow, C.
    Nichols, D.
    Nissanke, S.
    Nugent, P.
    Ofek, E.
    Qi, H.
    Quimby, R.
    Rosswog, S.
    Rusu, F.
    Sadler, E.
    Schmidt, P.
    Sollerman, J.
    Steele, I.
    Williamson, A.
    Xu, Y.
    Yan, L.
    Yatsu, Y.
    Zhang, C.
    Zhao, W.
    Date
    2017
    Type
    Journal Article
    
    Metadata
    Show full item record
    Citation
    Kasliwal, M. and Nakar, E. and Singer, L. and Kaplan, D. and Cook, D. and Van Sistine, A. and Lau, R. et al. 2017. Illuminating gravitational waves: A concordant picture of photons from a neutron star merger. Science. 358 (6370): pp. 1559-1565.
    Source Title
    Science
    DOI
    10.1126/science.aap9455
    ISSN
    0036-8075
    School
    Curtin Institute of Radio Astronomy (Physics)
    URI
    http://hdl.handle.net/20.500.11937/69473
    Collection
    • Curtin Research Publications
    Abstract

    Merging neutron stars offer an excellent laboratory for simultaneously studying strong-field gravity and matter in extreme environments. We establish the physical association of an electromagnetic counterpart (EM170817) with gravitational waves (GW170817) detected from merging neutron stars. By synthesizing a panchromatic data set, we demonstrate that merging neutron stars are a long-sought production site forging heavy elements by r-process nucleosynthesis. The weak gamma rays seen in EM170817 are dissimilar to classical short gamma-ray bursts with ultrarelativistic jets. Instead, we suggest that breakout of a wide-angle, mildly relativistic cocoon engulfing the jet explains the low-luminosity gamma rays, the high-luminosity ultraviolet-optical-infrared, and the delayed radio and x-ray emission. We posit that all neutron star mergers may lead to a wide-angle cocoon breakout, sometimes accompanied by a successful jet and sometimes by a choked jet.

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