Sökning: WFRF:(Gottlieb C) > Illuminating gravit...
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000 | 05448naa a2201261 4500 | |
001 | oai:DiVA.org:su-151196 | |
003 | SwePub | |
008 | 180111s2017 | |||||||||||000 ||eng| | |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-1511962 URI |
024 | 7 | a https://doi.org/10.1126/science.aap94552 DOI |
040 | a (SwePub)su | |
041 | a engb eng | |
042 | 9 SwePub | |
072 | 7 | a ref2 swepub-contenttype |
072 | 7 | a art2 swepub-publicationtype |
100 | 1 | a Kasliwal, M. M.4 aut |
245 | 1 0 | a Illuminating gravitational waves :b A concordant picture of photons from a neutron star merger |
264 | 1 | b American Association for the Advancement of Science (AAAS),c 2017 |
338 | a print2 rdacarrier | |
520 | a 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. | |
650 | 7 | a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng |
700 | 1 | a Nakar, E.4 aut |
700 | 1 | a Singer, L. P.4 aut |
700 | 1 | a Kaplan, D. L.4 aut |
700 | 1 | a Cook, D. O.4 aut |
700 | 1 | a Van Sistine, A.4 aut |
700 | 1 | a Lau, R. M.4 aut |
700 | 1 | a Fremling, C.4 aut |
700 | 1 | a Gottlieb, O.4 aut |
700 | 1 | a Jencson, J. E.4 aut |
700 | 1 | a Adams, S. M.4 aut |
700 | 1 | a Feindt, Ulrichu Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)ufein |
700 | 1 | a Hotokezaka, K.4 aut |
700 | 1 | a Ghosh, S.4 aut |
700 | 1 | a Perley, D. A.4 aut |
700 | 1 | a Yu, P-C.4 aut |
700 | 1 | a Piran, T.4 aut |
700 | 1 | a Allison, J. R.4 aut |
700 | 1 | a Anupama, G. C.4 aut |
700 | 1 | a Balasubramanian, A.4 aut |
700 | 1 | a Bannister, K. W.4 aut |
700 | 1 | a Bally, J.4 aut |
700 | 1 | a Barnes, J.4 aut |
700 | 1 | a Barway, S.4 aut |
700 | 1 | a Bellm, E.4 aut |
700 | 1 | a Bhalerao, V.4 aut |
700 | 1 | a Bhattacharya, D.4 aut |
700 | 1 | a Blagorodnova, N.4 aut |
700 | 1 | a Bloom, J. S.4 aut |
700 | 1 | a Brady, P. R.4 aut |
700 | 1 | a Cannella, C.4 aut |
700 | 1 | a Chatterjee, D.4 aut |
700 | 1 | a Cenko, S. B.4 aut |
700 | 1 | a Cobb, B. E.4 aut |
700 | 1 | a Copperwheat, C.4 aut |
700 | 1 | a Corsi, A.4 aut |
700 | 1 | a De, K.4 aut |
700 | 1 | a Dobie, D.4 aut |
700 | 1 | a Emery, S. W. K.4 aut |
700 | 1 | a Evans, P. A.4 aut |
700 | 1 | a Fox, O. D.4 aut |
700 | 1 | a Frail, D. A.4 aut |
700 | 1 | a Frohmaier, C.4 aut |
700 | 1 | a Goobar, Arielu Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)ariel |
700 | 1 | a Hallinan, G.4 aut |
700 | 1 | a Harrison, F.4 aut |
700 | 1 | a Helou, G.4 aut |
700 | 1 | a Hinderer, T.4 aut |
700 | 1 | a Ho, A. Y. Q.4 aut |
700 | 1 | a Horesh, A.4 aut |
700 | 1 | a Ip, W-H.4 aut |
700 | 1 | a Itoh, R.4 aut |
700 | 1 | a Kasen, D.4 aut |
700 | 1 | a Kim, H.4 aut |
700 | 1 | a Kuin, N. P. M.4 aut |
700 | 1 | a Kupfer, T.4 aut |
700 | 1 | a Lynch, C.4 aut |
700 | 1 | a Madsen, K.4 aut |
700 | 1 | a Mazzali, P. A.4 aut |
700 | 1 | a Miller, A. A.4 aut |
700 | 1 | a Mooley, K.4 aut |
700 | 1 | a Murphy, T.4 aut |
700 | 1 | a Ngeow, C-C.4 aut |
700 | 1 | a Nichols, D.4 aut |
700 | 1 | a Nissanke, S.4 aut |
700 | 1 | a Nugent, P.4 aut |
700 | 1 | a Ofek, E. O.4 aut |
700 | 1 | a Qi, H.4 aut |
700 | 1 | a Quimby, R. M.4 aut |
700 | 1 | a Rosswog, Stephanu Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)stero |
700 | 1 | a Rusu, F.4 aut |
700 | 1 | a Sadler, E. M.4 aut |
700 | 1 | a Schmidt, P.4 aut |
700 | 1 | a Sollerman, Jesperu Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)solle |
700 | 1 | a Steele, I.4 aut |
700 | 1 | a Williamson, A. R.4 aut |
700 | 1 | a Xu, Y.4 aut |
700 | 1 | a Yan, L.4 aut |
700 | 1 | a Yatsu, Y.4 aut |
700 | 1 | a Zhang, C.4 aut |
700 | 1 | a Zhao, W.4 aut |
710 | 2 | a Stockholms universitetb Fysikum4 org |
773 | 0 | t Scienced : American Association for the Advancement of Science (AAAS)g 358:6370, s. 1559-+q 358:6370<1559-+x 0036-8075x 1095-9203 |
856 | 4 | u https://arxiv.org/abs/1710.05436y arXiv:1710.05436 |
856 | 4 | u https://arxiv.org/pdf/1710.05436 |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-151196 |
856 | 4 8 | u https://doi.org/10.1126/science.aap9455 |
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