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Page 1
Electromagnetic evidence that SSS17a is the result of a binary neutron star merger.
Kilpatrick CD, Foley RJ, Kasen D, Murguia-Berthier A, Ramirez-Ruiz E, Coulter DA, Drout MR, Piro AL, Shappee BJ, Boutsia K, Contreras C, Di Mille F, Madore BF, Morrell N, Pan YC, Prochaska JX, Rest A, Rojas-Bravo C, Siebert MR, Simon JD, Ulloa N. Kilpatrick CD, et al. Among authors: di mille f. Science. 2017 Dec 22;358(6370):1583-1587. doi: 10.1126/science.aaq0073. Epub 2017 Oct 16. Science. 2017. PMID: 29038369
Early spectra of the gravitational wave source GW170817: Evolution of a neutron star merger.
Shappee BJ, Simon JD, Drout MR, Piro AL, Morrell N, Prieto JL, Kasen D, Holoien TW, Kollmeier JA, Kelson DD, Coulter DA, Foley RJ, Kilpatrick CD, Siebert MR, Madore BF, Murguia-Berthier A, Pan YC, Prochaska JX, Ramirez-Ruiz E, Rest A, Adams C, Alatalo K, Bañados E, Baughman J, Bernstein RA, Bitsakis T, Boutsia K, Bravo JR, Di Mille F, Higgs CR, Ji AP, Maravelias G, Marshall JL, Placco VM, Prieto G, Wan Z. Shappee BJ, et al. Among authors: di mille f. Science. 2017 Dec 22;358(6370):1574-1578. doi: 10.1126/science.aaq0186. Epub 2017 Oct 16. Science. 2017. PMID: 29038374
Light curves of the neutron star merger GW170817/SSS17a: Implications for r-process nucleosynthesis.
Drout MR, Piro AL, Shappee BJ, Kilpatrick CD, Simon JD, Contreras C, Coulter DA, Foley RJ, Siebert MR, Morrell N, Boutsia K, Di Mille F, Holoien TW, Kasen D, Kollmeier JA, Madore BF, Monson AJ, Murguia-Berthier A, Pan YC, Prochaska JX, Ramirez-Ruiz E, Rest A, Adams C, Alatalo K, Bañados E, Baughman J, Beers TC, Bernstein RA, Bitsakis T, Campillay A, Hansen TT, Higgs CR, Ji AP, Maravelias G, Marshall JL, Bidin CM, Prieto JL, Rasmussen KC, Rojas-Bravo C, Strom AL, Ulloa N, Vargas-González J, Wan Z, Whitten DD. Drout MR, et al. Among authors: di mille f. Science. 2017 Dec 22;358(6370):1570-1574. doi: 10.1126/science.aaq0049. Epub 2017 Oct 16. Science. 2017. PMID: 29038375
Periodic emission from the gamma-ray binary 1FGL J1018.6-5856.
Fermi LAT Collaboration, Ackermann M, Ajello M, Ballet J, Barbiellini G, Bastieri D, Belfiore A, Bellazzini R, Berenji B, Blandford RD, Bloom ED, Bonamente E, Borgland AW, Bregeon J, Brigida M, Bruel P, Buehler R, Buson S, Caliandro GA, Cameron RA, Caraveo PA, Cavazzuti E, Cecchi C, Çelik Ö, Charles E, Chaty S, Chekhtman A, Cheung CC, Chiang J, Ciprini S, Claus R, Cohen-Tanugi J, Corbel S, Corbet RH, Cutini S, de Luca A, den Hartog PR, de Palma F, Dermer CD, Digel SW, do Couto e Silva E, Donato D, Drell PS, Drlica-Wagner A, Dubois R, Dubus G, Favuzzi C, Fegan SJ, Ferrara EC, Focke WB, Fortin P, Fukazawa Y, Funk S, Fusco P, Gargano F, Gasparrini D, Gehrels N, Germani S, Giglietto N, Giordano F, Giroletti M, Glanzman T, Godfrey G, Grenier IA, Grove JE, Guiriec S, Hadasch D, Hanabata Y, Harding AK, Hayashida M, Hays E, Hill AB, Hughes RE, Jóhannesson G, Johnson AS, Johnson TJ, Kamae T, Katagiri H, Kataoka J, Kerr M, Knödlseder J, Kuss M, Lande J, Longo F, Loparco F, Lovellette MN, Lubrano P, Mazziotta MN, McEnery JE, Michelson PF, Mitthumsiri W, Mizuno T, Monte C, Monzani ME, Morselli A, Moskalenko IV, Murgia S, Nakamori T, Naumann-Godo M, Norris JP, Nuss E, Ohno M, Ohsugi T, Okumura… See abstract for full author list ➔ Fermi LAT Collaboration, et al. Among authors: di mille f. Science. 2012 Jan 13;335(6065):189-93. doi: 10.1126/science.1213974. Science. 2012. PMID: 22246769 Free article.