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Research output: Contribution to Journal/Magazine › Journal article › peer-review
Research output: Contribution to Journal/Magazine › Journal article › peer-review
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TY - JOUR
T1 - Heavy element production in a compact object merger observed by JWST
AU - Levan, Andrew
AU - Gompertz, Benjamin P.
AU - Salafia, Om Sharan
AU - Bulla, Mattia
AU - Burns, Eric
AU - Hotokezaka, Kenta
AU - Izzo, Luca
AU - Lamb, Gavin P.
AU - Malesani, Daniele B.
AU - Oates, Samantha R.
AU - Ravasio, Maria Edvige
AU - Escorial, Alicia Rouco
AU - Schneider, Benjamin
AU - Sarin, Nikhil
AU - Schulze, Steve
AU - Tanvir, Nial R.
AU - Ackley, Kendall
AU - Anderson, Gemma
AU - Brammer, Gabriel B.
AU - Christensen, Lise
AU - Dhillon, Vikram S.
AU - Evans, Phil A.
AU - Fausnaugh, Michael
AU - Fong, Wen-fai
AU - Fruchter, Andrew S.
AU - Fryer, Chris
AU - Fynbo, Johan P. U.
AU - Gaspari, Nicola
AU - Heintz, Kasper E.
AU - Hjorth, Jens
AU - Kennea, Jamie A.
AU - Kennedy, Mark R.
AU - Laskar, Tanmoy
AU - Leloudas, Giorgos
AU - Mandel, Ilya
AU - Martin-Carrillo, Antonio
AU - Metzger, Brian D.
AU - Nicholl, Matt
AU - Nugent, Anya
AU - Palmerio, Jesse T.
AU - Pugliese, Giovanna
AU - Rastinejad, Jillian
AU - Rhodes, Lauren
AU - Saccardi, Andrea
AU - Smartt, Stephen J.
AU - Stevance, Heloise F.
AU - Tohuvavohu, Aaron
AU - Horst, Alexander van der
AU - Vergani, Susanna D.
AU - Watson, Darach
AU - Barclay, Thomas
AU - Bhirombhakdi, Kornpob
AU - Breedt, Elmé
AU - Breeveld, Alice A.
AU - Brown, Alexander J.
AU - Campana, Sergio
AU - Chrimes, Ashley A.
AU - D’Avanzo, Paolo
AU - D’Elia, Valerio
AU - Pasquale, Massimiliano De
AU - Dyer, Martin J.
AU - Galloway, Duncan K.
AU - Garbutt, James A.
AU - Hartmann, Dieter H.
AU - Jakobsson, Páll
AU - Kerry, Paul
AU - Kouveliotou, Chryssa
AU - Langeroodi, Danial
AU - Floc’h, Emeric Le
AU - Leung, James K.
AU - Littlefair, Stuart P.
AU - Munday, James
AU - O’Brien, Paul
AU - Parsons, Steven G.
AU - Pelisoli, Ingrid
AU - Sahman, David I.
AU - Salvaterra, Ruben
AU - Sbarufatti, Boris
AU - Steeghs, Danny
AU - Tagliaferri, Gianpiero
AU - Thöne, Christina C.
AU - Postigo, Antonio de Ugarte
AU - Kann, David Alexander
PY - 2024/2/22
Y1 - 2024/2/22
N2 - The mergers of binary compact objects such as neutron stars and black holes are of central interest to several areas of astrophysics, including as the progenitors of gamma-ray bursts (GRBs) 1, sources of high-frequency gravitational waves (GWs) 2 and likely production sites for heavy-element nucleosynthesis by means of rapid neutron capture (the r-process) 3. Here we present observations of the exceptionally bright GRB 230307A. We show that GRB 230307A belongs to the class of long-duration GRBs associated with compact object mergers 4–6 and contains a kilonova similar to AT2017gfo, associated with the GW merger GW170817 (refs. 7–12). We obtained James Webb Space Telescope (JWST) mid-infrared imaging and spectroscopy 29 and 61 days after the burst. The spectroscopy shows an emission line at 2.15 microns, which we interpret as tellurium (atomic mass A = 130) and a very red source, emitting most of its light in the mid-infrared owing to the production of lanthanides. These observations demonstrate that nucleosynthesis in GRBs can create r-process elements across a broad atomic mass range and play a central role in heavy-element nucleosynthesis across the Universe.
AB - The mergers of binary compact objects such as neutron stars and black holes are of central interest to several areas of astrophysics, including as the progenitors of gamma-ray bursts (GRBs) 1, sources of high-frequency gravitational waves (GWs) 2 and likely production sites for heavy-element nucleosynthesis by means of rapid neutron capture (the r-process) 3. Here we present observations of the exceptionally bright GRB 230307A. We show that GRB 230307A belongs to the class of long-duration GRBs associated with compact object mergers 4–6 and contains a kilonova similar to AT2017gfo, associated with the GW merger GW170817 (refs. 7–12). We obtained James Webb Space Telescope (JWST) mid-infrared imaging and spectroscopy 29 and 61 days after the burst. The spectroscopy shows an emission line at 2.15 microns, which we interpret as tellurium (atomic mass A = 130) and a very red source, emitting most of its light in the mid-infrared owing to the production of lanthanides. These observations demonstrate that nucleosynthesis in GRBs can create r-process elements across a broad atomic mass range and play a central role in heavy-element nucleosynthesis across the Universe.
U2 - 10.1038/s41586-023-06759-1
DO - 10.1038/s41586-023-06759-1
M3 - Journal article
VL - 626
SP - 737
EP - 741
JO - Nature
JF - Nature
SN - 0028-0836
ER -