Sökning: WFRF:(Siegel J) > (2015-2019) > Swift and NuSTAR ob...
Fältnamn | Indikatorer | Metadata |
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000 | 04350naa a2200985 4500 | |
001 | oai:DiVA.org:su-151197 | |
003 | SwePub | |
008 | 180111s2017 | |||||||||||000 ||eng| | |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-1511972 URI |
024 | 7 | a https://doi.org/10.1126/science.aap95802 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 Evans, P. A.4 aut |
245 | 1 0 | a Swift and NuSTAR observations of GW170817 :b Detection of a blue kilonova |
264 | 1 | b American Association for the Advancement of Science (AAAS),c 2017 |
338 | a print2 rdacarrier | |
520 | a With the first direct detection of merging black holes in 2015, the era of gravitational wave (GW) astrophysics began. A complete picture of compact object mergers, however, requires the detection of an electromagnetic (EM) counterpart. We report ultraviolet (UV) and x-ray observations by Swift and the Nuclear Spectroscopic Telescope Array of the EM counter part of the binary neutron star merger GW170817. The bright, rapidly fading UV emission indicates a high mass (approximate to 0.03 solar masses) wind-driven outflow with moderate electron fraction (Y-e approximate to 0.27). Combined with the x-ray limits, we favor an observer viewing angle of approximate to 30 degrees away from the orbital rotation axis, which avoids both obscuration from the heaviest elements in the orbital plane and a direct view of any ultrarelativistic, highly collimated ejecta (a gamma-ray burst afterglow). | |
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 Cenko, S. B.4 aut |
700 | 1 | a Kennea, J. A.4 aut |
700 | 1 | a Emery, S. W. K.4 aut |
700 | 1 | a Kuin, N. P. M.4 aut |
700 | 1 | a Korobkin, O.4 aut |
700 | 1 | a Wollaeger, R. T.4 aut |
700 | 1 | a Fryer, C. L.4 aut |
700 | 1 | a Madsen, K. K.4 aut |
700 | 1 | a Harrison, F. A.4 aut |
700 | 1 | a Xu, Y.4 aut |
700 | 1 | a Nakar, E.4 aut |
700 | 1 | a Hotokezaka, K.4 aut |
700 | 1 | a Lien, A.4 aut |
700 | 1 | a Campana, S.4 aut |
700 | 1 | a Oates, S. R.4 aut |
700 | 1 | a Troja, E.4 aut |
700 | 1 | a Breeveld, A. A.4 aut |
700 | 1 | a Marshall, F. E.4 aut |
700 | 1 | a Barthelmy, S. D.4 aut |
700 | 1 | a Beardmore, A. P.4 aut |
700 | 1 | a Burrows, D. N.4 aut |
700 | 1 | a Cusumano, G.4 aut |
700 | 1 | a D'Ai, A.4 aut |
700 | 1 | a D'Avanzo, P.4 aut |
700 | 1 | a D'Elia, V.4 aut |
700 | 1 | a De Pasquale, M.4 aut |
700 | 1 | a Even, W. P.4 aut |
700 | 1 | a Fontes, C. J.4 aut |
700 | 1 | a Forster, K.4 aut |
700 | 1 | a Garcia, J.4 aut |
700 | 1 | a Giommi, P.4 aut |
700 | 1 | a Grefenstette, B.4 aut |
700 | 1 | a Gronwall, C.4 aut |
700 | 1 | a Hartmann, D. H.4 aut |
700 | 1 | a Heida, M.4 aut |
700 | 1 | a Hungerford, A. L.4 aut |
700 | 1 | a Kasliwal, M. M.4 aut |
700 | 1 | a Krimm, H. A.4 aut |
700 | 1 | a Levan, A. J.4 aut |
700 | 1 | a Malesani, D.4 aut |
700 | 1 | a Melandri, A.4 aut |
700 | 1 | a Miyasaka, H.4 aut |
700 | 1 | a Nousek, J. A.4 aut |
700 | 1 | a O'Brien, P. T.4 aut |
700 | 1 | a Osborne, J. P.4 aut |
700 | 1 | a Pagani, C.4 aut |
700 | 1 | a Page, K. L.4 aut |
700 | 1 | a Palmer, D. M.4 aut |
700 | 1 | a Perri, M.4 aut |
700 | 1 | a Pike, S.4 aut |
700 | 1 | a Racusin, J. L.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 Siegel, M. H.4 aut |
700 | 1 | a Sakamoto, T.4 aut |
700 | 1 | a Sbarufatti, B.4 aut |
700 | 1 | a Tagliaferri, G.4 aut |
700 | 1 | a Tanvir, N. R.4 aut |
700 | 1 | a Tohuvavohu, A.4 aut |
710 | 2 | a Stockholms universitetb Institutionen för astronomi4 org |
773 | 0 | t Scienced : American Association for the Advancement of Science (AAAS)g 358:6370, s. 1565-1569q 358:6370<1565-1569x 0036-8075x 1095-9203 |
856 | 4 | u https://authors.library.caltech.edu/82060/6/1710.05437.pdf |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-151197 |
856 | 4 8 | u https://doi.org/10.1126/science.aap9580 |
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