2017
Spectroscopic identification of r-process nucleosynthesis in a double neutron-star merger
Abstract: 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). Such transients, named 'macronovae' or 'kilonovae', are believed to be centres of production of rare elements such as gold and platinum. The most compelling evidence so far for a kilonova was a very faint near-inf…
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Cited by 1,086 publications
(776 citation statements)
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“…The deep upper limit from Gemini shows that at ~10 days the afterglow became the dominant component and the kilonova already faded away. This is consistent with the behavior of AT2017gfo 8 , 10 , 20 , and predicted in general by kilonova models 13 , 29 , 30 .…”
Section: Resultssupporting
confidence: 91%
“…The deep upper limit from Gemini shows that at ~10 days the afterglow became the dominant component and the kilonova already faded away. This is consistent with the behavior of AT2017gfo 8 , 10 , 20 , and predicted in general by kilonova models 13 , 29 , 30 .…”
Section: Resultssupporting
confidence: 91%
“…The light curves from our simulations have higher apparent magnitude compared to the previous results in Nativi et al ( 2021 ). The values presented in this paper are closer to the apparent magnitude observed for GW 170 817 KN AT2017gfo (Andreoni et al 2017 ;Arcavi et al 2017 ;Chornock et al 2017 ;Cowperthwaite et al 2017 ;Drout et al 2017 ;Evans et al 2017 ;Kasliwal et al 2017 ;Pian et al 2017 ;Smartt et al 2017 ;Tanvir et al 2017 ;Troja et al 2017 ;Utsumi et al 2017 ;Valenti et al 2017 ). In both cases, the variation with inclination angles is greatest for the Wind model.…”
Section: Discussion Ssupporting
confidence: 85%
“…5). This is consistent with previous findings suggesting that AT 2017gfo was observed at 15 • θ obs 30 • (0.87 cos θ obs 0.97) from the polar axis (Abbott et al 2017;Pian et al 2017;Troja et al 2017;Finstad et al 2018;Mandel 2018;Mooley et al 2018). The good agreement is especially true at bluer wavelengths (ugri).…”
Section: Broad-band Light Curvessupporting
confidence: 92%

