3 years ago

Spectroscopic identification of r-process nucleosynthesis in a double neutron-star merger

Spectroscopic identification of r-process nucleosynthesis in a double neutron-star merger
M. Turatto, A. Melandri, S. Covino, A. Stamerra, G. Greco, G. Tagliaferri, M. Razzano, N. R. Tanvir, M. Boër, M. Capaccioli, A. Bulgarelli, D. Watson, F. Getman, A. Levan, C. M. Copperwheat, G. Ghirlanda, S. Benetti, N. Masetti, M. Tanaka, F. Longo, G. Giuffrida, F. Bufano, E. Brocato, L. Stella, L. K. Hunt, S. Campana, R. Ciolfi, A. J. Castro-Tirado, C. Kouveliotou, T. Piran, P. Møller, P. Schipani, L. Pulone, M. Spera, G. Stratta, E. Maiorano, L. Nicastro, V. D’Elia, R. Salvaterra, S. Yang, O. S. Salafia, S. Piranomonte, J. Hjorth, A. Grado, S. Klose, P. Casella, J. Selsing, L. Nava, A. Di Paola, M. Dadina, A. Rossi, M. M. Kasliwal, D. Vergani, J. P. U. Fynbo, D. Malesani, G. Ghisellini, A. Giunta, E. Palazzi, G. De Cesare, M. Lisi, E. Chassande-Mottin, E. Cappellaro, B. Patricelli, L. Amati, A. Pescalli, G. L. Israel, A. Possenti, L. A. Antonelli, P. A. Mazzali, E. Pian, D. Perley, M. Branchesi, B. Gendre, M. G. Bernardini, Z.-P. Jin, E. Troja, V. Testa, L. Limatola, S. D. Vergani, Y. Z. Fan, P. D’Avanzo, M. Mapelli, S. Ascenzi, L. Tomasella

The merger of two neutron stars is predicted to give rise to three major detectable phenomena: a short burst of γ-rays, a gravitational-wave signal, and a transient optical–near-infrared source powered by the synthesis of large amounts of very heavy elements via rapid neutron capture (the r-process)1,2,3. Such transients, named ‘macronovae’ or ‘kilonovae’4,5,6,7, are believed to be centres of production of rare elements such as gold and platinum8. The most compelling evidence so far for a kilonova was a very faint near-infrared rebrightening in the afterglow of a short γ-ray burst9,10 at redshift z = 0.356, although findings indicating bluer events have been reported11. Here we report the spectral identification and describe the physical properties of a bright kilonova associated with the gravitational-wave source12 GW170817 and γ-ray burst13,14 GRB 170817A associated with a galaxy at a distance of 40 megaparsecs from Earth. Using a series of spectra from ground-based observatories covering the wavelength range from the ultraviolet to the near-infrared, we find that the kilonova is characterized by rapidly expanding ejecta with spectral features similar to those predicted by current models15,16. The ejecta is optically thick early on, with a velocity of about 0.2 times light speed, and reaches a radius of about 50 astronomical units in only 1.5 days. As the ejecta expands, broad absorption-like lines appe

-Abstract Truncated-

Publisher URL: http://dx.doi.org/10.1038/nature24298

DOI: 10.1038/nature24298

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