Abstract
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 (GW)2 and likely production sites for heavy element nucleosynthesis via rapid neutron capture (the r-process)3. Here we present observations of the exceptionally bright gamma-ray burst GRB 230307A. We show that GRB 230307A belongs to the class of long-duration gamma-ray bursts associated with compact object mergers4–6, and contains a kilonova similar to AT2017gfo, associated with the gravitational-wave merger GW1708177–12. We obtained James Webb Space Telescope mid-infrared (mid-IR) 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-IR due 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.
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Supplementary information
Supplementary Information
The Supplementary Information contains further discussion relevant to the nature and properties of GRB 230307A. In particular, we place the burst properties in context with those of other GRBs in both the prompt (SI 1.1) and afterglow regimes (SI 1.2). We also provide further details regarding identifying the host galaxy and its detailed properties in SI 1.3 and 1.4. SI 1.5 considers the extreme brightness of the burst and investigates similarities and differences with other very bright GRBs. In SI 2, we consider the inferred event rates for bursts like GRB 230307A. SI 3 provides additional details regarding modelling the light curve (SI 3.1) and spectrum (SI 3.2). Finally, SI 4 investigates a broad range of alternative progenitor possibilities and their challenges and a justification for our chosen interpretation. This includes the high-z case (SI 4.1), lower redshift supernovae (SI 4.2 and 4.3), Galactic sources (SI 4.4) and white dwarf – neutron star mergers (SI 4.5). Supplementary figures and tables are also provided as referenced in both the main text, methods and supplementary information.
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Levan, A., Gompertz, B.P., Salafia, O.S. et al. Heavy element production in a compact object merger observed by JWST.
Nature (2023). https://doi.org/10.1038/s41586-023-06759-1
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Received: 03 July 2023
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Accepted: 17 October 2023
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Published: 25 October 2023
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DOI: https://doi.org/10.1038/s41586-023-06759-1
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