A lanthanide-rich kilonova in the aftermath of a long gamma-ray burst.


Journal

Nature
ISSN: 1476-4687
Titre abrégé: Nature
Pays: England
ID NLM: 0410462

Informations de publication

Date de publication:
Feb 2024
Historique:
received: 31 07 2023
accepted: 14 12 2023
medline: 22 2 2024
pubmed: 22 2 2024
entrez: 21 2 2024
Statut: ppublish

Résumé

Observationally, kilonovae are astrophysical transients powered by the radioactive decay of nuclei heavier than iron, thought to be synthesized in the merger of two compact objects

Identifiants

pubmed: 38383623
doi: 10.1038/s41586-023-06979-5
pii: 10.1038/s41586-023-06979-5
doi:

Types de publication

Journal Article

Langues

eng

Sous-ensembles de citation

IM

Pagination

742-745

Informations de copyright

© 2024. The Author(s), under exclusive licence to Springer Nature Limited.

Références

Eichler, D., Livio, M., Piran, T. & Schramm, D. N. Nucleosynthesis, neutrino bursts and γ-rays from coalescing neutron stars. Nature 340, 126–128 (1989).
doi: 10.1038/340126a0
Li, L.-X. & Paczyński, B. Transient events from neutron star mergers. Astrophys. J. 507, L59–L62 (1998).
doi: 10.1086/311680
Freiburghaus, C., Rosswog, S. & Thielemann, F. K. R-process in neutron star mergers. Astrophys. J. 525, L121–L124 (1999).
pubmed: 10525469 doi: 10.1086/312343
Korobkin, O., Rosswog, S., Arcones, A. & Winteler, C. On the astrophysical robustness of the neutron star merger r-process. Mon. Not. R. Astron. Soc. 426, 1940–1949 (2012).
doi: 10.1111/j.1365-2966.2012.21859.x
Barnes, J., Kasen, D., Wu, M.-R. & Martínez-Pinedo, G. Radioactivity and thermalization in the ejecta of compact object mergers and their impact on kilonova light curves. Astrophys. J. 829, 110 (2016).
doi: 10.3847/0004-637X/829/2/110
Hotokezaka, K. & Nakar, E. Radioactive heating rate of r-process elements and macronova light curve. Astrophys. J. 891, 152 (2020).
doi: 10.3847/1538-4357/ab6a98
Zhu, J.-P. et al. Long-duration gamma-ray burst and associated kilonova emission from fast-spinning black hole–neutron star mergers. Astrophys. J. 936, L10 (2022).
doi: 10.3847/2041-8213/ac85ad
Wollaeger, R. T. et al. Impact of pulsar and fallback sources on multifrequency kilonova models. Astrophys. J. 880, 22 (2019).
doi: 10.3847/1538-4357/ab25f5
Levan, A. et al. Heavy element production in a compact object merger observed by JWST. Nature https://doi.org/10.1038/s41586-023-06759-1 (2023).
Sun, H. et al. Magnetar emergence in a peculiar gamma-ray burst from a compact star merger. Preprint at https://arxiv.org/abs/2307.05689 (2023).
Bloom, J. S., Kulkarni, S. R. & Djorgovski, S. G. The observed offset distribution of gamma-ray bursts from their host galaxies: a robust clue to the nature of the progenitors. Astron. J. 123, 1111–1148 (2002).
doi: 10.1086/338893
Freedman, W. L. et al. The Carnegie-Chicago Hubble Program. VIII. An independent determination of the Hubble constant based on the tip of the red giant branch. Astrophys. J. 882, 34 (2019).
doi: 10.3847/1538-4357/ab2f73
Waxman, E., Ofek, E. O. & Kushnir, D. Late-time kilonova light curves and implications to GW170817. Astrophys. J. 878, 93 (2019).
doi: 10.3847/1538-4357/ab1f71
Kasliwal, M. M. et al. Spitzer mid-infrared detections of neutron star merger GW170817 suggests synthesis of the heaviest elements. Mon. Not. R. Astron. Soc. 510, L7–L12 (2022).
doi: 10.1093/mnrasl/slz007
Troja, E. et al. A nearby long gamma-ray burst from a merger of compact objects. Nature 612, 228–231 (2022).
pubmed: 36477127 pmcid: 9729102 doi: 10.1038/s41586-022-05327-3
Gehrels, N. et al. A new γ-ray burst classification scheme from GRB060614. Nature 444, 1044–1046 (2006).
pubmed: 17183315 doi: 10.1038/nature05376
Yang, B. et al. A possible macronova in the late afterglow of the long-short burst GRB 060614. Nat. Commun. 6, 7323 (2015).
pubmed: 26065563 doi: 10.1038/ncomms8323
Jin, Z.-P. et al. The light curve of the macronova associated with the long-short burst GRB 060614. Astrophys. J. 811, L22 (2015).
doi: 10.1088/2041-8205/811/2/L22
Rastinejad, J. C. et al. A kilonova following a long-duration gamma-ray burst at 350 Mpc. Nature 612, 223–227 (2022).
pubmed: 36477128 doi: 10.1038/s41586-022-05390-w
Yang, J. et al. A long-duration gamma-ray burst with a peculiar origin. Nature 612, 232–235 (2022).
pubmed: 36477130 doi: 10.1038/s41586-022-05403-8
Ryan, G., van Eerten, H., Piro, L. & Troja, E. Gamma-ray burst afterglows in the multimessenger era: numerical models and closure relations. Astrophys. J. 896, 166 (2020).
doi: 10.3847/1538-4357/ab93cf
Valenti, S. et al. The diversity of type II supernova versus the similarity in their progenitors. Mon. Not. R. Astron. Soc. 459, 3939–3962 (2016).
doi: 10.1093/mnras/stw870
Barnes, J. et al. Kilonovae across the nuclear physics landscape: the impact of nuclear physics uncertainties on r-process-powered emission. Astrophys. J. 918, 44 (2021).
doi: 10.3847/1538-4357/ac0aec
Frey, L. H. et al. The Los Alamos Supernova Light-curve Project: computational methods. Astrophys. J. 204, 16 (2013).
doi: 10.1088/0067-0049/204/2/16
Fontes, C. J., Fryer, C. L., Hungerford, A. L., Wollaeger, R. T. & Korobkin, O. A line-binned treatment of opacities for the spectra and light curves from neutron star mergers. Mon. Not. R. Astron. Soc. 493, 4143–4171 (2020).
doi: 10.1093/mnras/staa485
Fontes, C. J., Fryer, C. L., Wollaeger, R. T., Mumpower, M. R. & Sprouse, T. M. Actinide opacities for modelling the spectra and light curves of kilonovae. Mon. Not. R. Astron. Soc. 519, 2862–2878 (2023).
doi: 10.1093/mnras/stac2792
Zhu, Y. et al. Californium-254 and kilonova light curves. Astrophys. J. 863, L23 (2018).
doi: 10.3847/2041-8213/aad5de
Holmbeck, E. M. et al. Superheavy elements in kilonovae. Astrophys. J. 951, L13 (2023).
doi: 10.3847/2041-8213/acd9cb
Waxman, E., Ofek, E. O., Kushnir, D. & Gal-Yam, A. Constraints on the ejecta of the GW170817 neutron star merger from its electromagnetic emission. Mon. Not. R. Astron. Soc. 481, 3423–3441 (2018).
doi: 10.1093/mnras/sty2441
Arnaud, K. A. XSPEC: the first ten years. In Astronomical Data Analysis Software and Systems V, Conference Series Vol. 101 (eds Jacoby, G. H. & Barnes, J.) 17–20 (Astronomical Society of the Pacific, 1996).
Willingale, R., Starling, R. L. C., Beardmore, A. P., Tanvir, N. R. & O’Brien, P. T. Calibration of X-ray absorption in our Galaxy. Mon. Not. R. Astron. Soc. 431, 394–404 (2013).
doi: 10.1093/mnras/stt175
Schlafly, E. F. & Finkbeiner, D. P. Measuring reddening with Sloan Digital Sky Survey stellar spectra and recalibrating SFD. Astrophys. J. 737, 103 (2011).
doi: 10.1088/0004-637X/737/2/103
Waxman, E., Ofek, E. O. & Kushnir, D. Strong NIR emission following the long duration GRB 211211A: dust heating as an alternative to a kilonova. Preprint at https://arxiv.org/abs/2206.10710 (2022).
Krühler, T. et al. The SEDs and host galaxies of the dustiest GRB afterglows. Astron. Astrophys. 534, A108 (2011).
doi: 10.1051/0004-6361/201117428
Sneppen, A. et al. Spherical symmetry in the kilonova AT2017gfo/GW170817. Nature 614, 436–439 (2023).
pubmed: 36792736 doi: 10.1038/s41586-022-05616-x
Levan, A. J. et al. GRB 230307A: JWST NIRSpec observations, possible higher redshift. GRB Coord. Netw. Circ. No. 33580 (2023).
Windhorst, R. A. et al. JWST PEARLS. Prime Extragalactic Areas for Reionization and Lensing Science: project overview and first results. Astron. J. 165, 13 (2023).
doi: 10.3847/1538-3881/aca163
Chang, H.-Y. & Kim, H.-I. On spatial distribution of short gamma-ray bursts from extragalactic magnetar flares. J. Astron. Space Sci. 19, 1–6 (2002).
doi: 10.5140/JASS.2002.19.1.001
Dichiara, S. et al. A luminous precursor in the extremely bright GRB 230307A. Astrophys. J. 954, L29 (2023).
doi: 10.3847/2041-8213/acf21d
Yang, J. et al. GRB 200415A: a short gamma-ray burst from a magnetar giant flare? Astrophys. J. 899, 106 (2020).
doi: 10.3847/1538-4357/aba745
Wang, Y., Xia, Z.-Q., Zheng, T.-C., Ren, J. & Fan, Y.-Z. A broken “α–intensity” relation caused by the evolving photosphere emission and the nature of the extraordinarily bright GRB 230307A. Astrophys. J. 953, L8 (2023).
doi: 10.3847/2041-8213/ace7d4
Planck Collaboration et al. Planck 2018 results. VI. Cosmological parameters. Astron. Astrophys. 641, A6 (2020).
doi: 10.1051/0004-6361/201833910
O’Connor, B. et al. A deep survey of short GRB host galaxies over z ~ 0–2: implications for offsets, redshifts, and environments. Mon. Not. R. Astron. Soc. 515, 4890–4928 (2022).
doi: 10.1093/mnras/stac1982
Jin, Z.-P. et al. A kilonova associated with GRB 070809. Nat. Astron. 4, 77–82 (2020).
doi: 10.1038/s41550-019-0892-y
O’Connor, B., Beniamini, P. & Kouveliotou, C. Constraints on the circumburst environments of short gamma-ray bursts. Mon. Not. R. Astron. Soc. 495, 4782–4799 (2020).
doi: 10.1093/mnras/staa1433
Norris, J. P. & Bonnell, J. T. Short gamma-ray bursts with extended emission. Astrophys. J. 643, 266–275 (2006).
doi: 10.1086/502796
Dichiara, S. et al. Evidence of extended emission in GRB 181123B and other high-redshift short GRBs. Astrophys. J. 911, L28 (2021).
doi: 10.3847/2041-8213/abf562
Kennicutt, J. & Robert, C. Star formation in galaxies along the Hubble sequence. Ann. Rev. Astron. Astrophys. 36, 189–232 (1998).
doi: 10.1146/annurev.astro.36.1.189
Chabrier, G. Galactic stellar and substellar initial mass function. Publ. Astron. Soc. Pac. 115, 763–795 (2003).
doi: 10.1086/376392
Kobulnicky, H. A. & Kewley, L. J. Metallicities of 0.3<z<1.0 galaxies in the GOODS-North field. Astrophys. J. 617, 240–261 (2004).
doi: 10.1086/425299
Johnson, B. D., Leja, J., Conroy, C. & Speagle, J. S. Stellar population inference with Prospector. Astrophys. J. 254, 22 (2021).
doi: 10.3847/1538-4365/abef67
O’Connor, B. et al. A tale of two mergers: constraints on kilonova detection in two short GRBs at z ~ 0.5. Mon. Not. R. Astron. Soc. 502, 1279–1298 (2021).
Palmerio, J. T. et al. Are long gamma-ray bursts biased tracers of star formation? Clues from the host galaxies of the Swift/BAT6 complete sample of bright LGRBs. III. Stellar masses, star formation rates, and metallicities at z > 1. Astron. Astrophys. 623, A26 (2019).
doi: 10.1051/0004-6361/201834179
Whitaker, K. E., van Dokkum, P. G., Brammer, G. & Franx, M. The star formation mass sequence out to z = 2.5. Astrophys. J. 754, L29 (2012).
doi: 10.1088/2041-8205/754/2/L29
Amati, L. et al. Intrinsic spectra and energetics of BeppoSAX gamma-ray bursts with known redshifts. Astron. Astrophys. 390, 81–89 (2002).
doi: 10.1051/0004-6361:20020722
O’Connor, B. et al. A structured jet explains the extreme GRB 221009a. Sci. Adv. 9, eadi1405 (2023).
pubmed: 37285439 pmcid: 10246904 doi: 10.1126/sciadv.adi1405
Kouveliotou, C. et al. Identification of two classes of gamma-ray bursts. Astrophys. J. 413, L101 (1993).
doi: 10.1086/186969
Becerra, R. L. et al. Deciphering the unusual stellar progenitor of GRB 210704A. Mon. Not. R. Astron. Soc. 522, 5204–5216 (2023).
doi: 10.1093/mnras/stad1372
Clocchiatti, A., Suntzeff, N. B., Covarrubias, R. & Candia, P. The ultimate light curve of SN 1998bw/GRB 980425. Astron. J. 141, 163 (2011).
doi: 10.1088/0004-6256/141/5/163
Srinivasaragavan, G. P. et al. A sensitive search for supernova emission associated with the extremely energetic and nearby GRB 221009A. Astrophys. J. 949, L39 (2023).
doi: 10.3847/2041-8213/accf97
Perets, H. B. et al. A faint type of supernova from a white dwarf with a helium-rich companion. Nature 465, 322–325 (2010).
pubmed: 20485429 doi: 10.1038/nature09056
Kasliwal, M. M. et al. Rapidly decaying supernova 2010X: a candidate “.Ia” explosion. Astrophys. J. 723, L98–L102 (2010).
doi: 10.1088/2041-8205/723/1/L98
Zhong, S.-Q., Li, L. & Dai, Z.-G. GRB 211211A: a neutron star-white dwarf merger? Astrophys. J. 947, L21 (2023).
doi: 10.3847/2041-8213/acca83
Fryer, C. L., Woosley, S. E., Herant, M. & Davies, M. B. Merging white dwarf/black hole binaries and gamma-ray bursts. Astrophys. J. 520, 650–660 (1999).
doi: 10.1086/307467
Kaltenborn, M. A. R. et al. Abundances and transients from neutron star-white dwarf mergers. Astrophys. J. 956, 71 (2023).
doi: 10.3847/1538-4357/acf860
Bobrick, A., Zenati, Y., Perets, H. B., Davies, M. B. & Church, R. Transients from one white dwarf–neutron star/black hole mergers. Mon. Not. R. Astron. Soc. 510, 3758–3777 (2022).
doi: 10.1093/mnras/stab3574
Lu, W. & Quataert, E. Late-time accretion in neutron star mergers: implications for short gamma-ray bursts and kilonovae. Mon. Not. R. Astron. Soc. 522, 5848–5861 (2023).
doi: 10.1093/mnras/stad1336
Gao, H., Lei, W.-H., Zou, Y.-C., Wu, X.-F. & Zhang, B. A complete reference of the analytical synchrotron external shock models of gamma-ray bursts. New Astron. Rev. 57, 141–190 (2013).
doi: 10.1016/j.newar.2013.10.001
Metzger, B. D. Kilonovae. Living Rev. Relativ. 23, 1 (2019).
pubmed: 31885490 pmcid: 6914724 doi: 10.1007/s41114-019-0024-0
Buchner, J. et al. X-ray spectral modelling of the AGN obscuring region in the CDFS: Bayesian model selection and catalogue. Astron. Astrophys. 564, A125 (2014).
doi: 10.1051/0004-6361/201322971
Mereghetti, S., Rigoselli, M., Salvaterra, R., Tiengo, A. & Pacholski, D. P. XMM-Newton and INTEGRAL observations of the bright GRB 230307A: vanishing of the local absorption and limits on the dust in the Magellanic Bridge. Astrophys. J. 956, 97 (2023).
doi: 10.3847/1538-4357/acf846
Zhang, B. & Mészáros, P. Gamma-ray bursts: progress, problems & prospects. Int. J. Mod. Phys. A 19, 2385–2472 (2004).
doi: 10.1142/S0217751X0401746X

Auteurs

Yu-Han Yang (YH)

Department of Physics, University of Rome "Tor Vergata", Rome, Italy. yuhan.yang@roma2.infn.it.

Eleonora Troja (E)

Department of Physics, University of Rome "Tor Vergata", Rome, Italy. eleonora.troja@uniroma2.it.
INAF - Istituto Nazionale di Astrofisica, Rome, Italy. eleonora.troja@uniroma2.it.

Brendan O'Connor (B)

Department of Physics, The George Washington University, Washington DC, USA.
Department of Astronomy, University of Maryland, College Park, MD, USA.
Astrophysics Science Division, NASA Goddard Space Flight Center, Greenbelt, MD, USA.

Chris L Fryer (CL)

Computer, Computational, and Statistical Sciences Division, Los Alamos National Laboratory, Los Alamos, NM, USA.
Center for Theoretical Astrophysics, Los Alamos National Laboratory, Los Alamos, NM, USA.
The University of Arizona, Tucson, AZ, USA.
Department of Physics and Astronomy, The University of New Mexico, Albuquerque, NM, USA.
The George Washington University, Washington DC, USA.

Myungshin Im (M)

SNU Astronomy Research Center, Astronomy Program, Department of Physics and Astronomy, Seoul National University, Seoul, Republic of Korea.

Joe Durbak (J)

Department of Astronomy, University of Maryland, College Park, MD, USA.
Astrophysics Science Division, NASA Goddard Space Flight Center, Greenbelt, MD, USA.

Gregory S H Paek (GSH)

SNU Astronomy Research Center, Astronomy Program, Department of Physics and Astronomy, Seoul National University, Seoul, Republic of Korea.

Roberto Ricci (R)

Istituto Nazionale di Ricerca Metrologica, Turin, Italy.
INAF - Istituto di Radioastronomia, Bologna, Italy.

Clécio R Bom (CR)

Centro Brasileiro de Pesquisas Físicas, Rio de Janeiro, Brazil.
Centro Federal de Educação Tecnológica Celso Suckow da Fonseca, Rodovia Mário Covas, Itaguaí, Brazil.

James H Gillanders (JH)

Department of Physics, University of Rome "Tor Vergata", Rome, Italy.

Alberto J Castro-Tirado (AJ)

Instituto de Astrofísica de Andalucía (IAA-CSIC), Granada, Spain.
Unidad Asociada al CSIC Departamento de Ingeniería de Sistemas y Automática, Escuela de Ingenierías Industriales, Universidad de Málaga, Málaga, Spain.

Zong-Kai Peng (ZK)

Institute for Frontier in Astronomy and Astrophysics, Beijing Normal University, Beijing, China.
Department of Astronomy, Beijing Normal University, Beijing, China.

Simone Dichiara (S)

Department of Astronomy and Astrophysics, The Pennsylvania State University, University Park, PA, USA.

Geoffrey Ryan (G)

Perimeter Institute for Theoretical Physics, Waterloo, Ontario, Canada.

Hendrik van Eerten (H)

Physics Department, University of Bath, Claverton Down, UK.

Zi-Gao Dai (ZG)

Department of Astronomy, School of Physical Sciences, University of Science and Technology of China, Hefei, China.

Seo-Won Chang (SW)

SNU Astronomy Research Center, Astronomy Program, Department of Physics and Astronomy, Seoul National University, Seoul, Republic of Korea.

Hyeonho Choi (H)

SNU Astronomy Research Center, Astronomy Program, Department of Physics and Astronomy, Seoul National University, Seoul, Republic of Korea.

Kishalay De (K)

Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA.

Youdong Hu (Y)

Instituto de Astrofísica de Andalucía (IAA-CSIC), Granada, Spain.

Charles D Kilpatrick (CD)

Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA) and Department of Physics and Astronomy, Northwestern University, Evanston, IL, USA.

Alexander Kutyrev (A)

Department of Astronomy, University of Maryland, College Park, MD, USA.
Astrophysics Science Division, NASA Goddard Space Flight Center, Greenbelt, MD, USA.

Mankeun Jeong (M)

SNU Astronomy Research Center, Astronomy Program, Department of Physics and Astronomy, Seoul National University, Seoul, Republic of Korea.

Chung-Uk Lee (CU)

Korea Astronomy and Space Science Institute, Daejeon, Republic of Korea.

Martin Makler (M)

Centro Brasileiro de Pesquisas Físicas, Rio de Janeiro, Brazil.
International Center for Advanced Studies and Instituto de Ciencias Físicas, ECyT-UNSAM and CONICET, Buenos Aires, Argentina.

Felipe Navarete (F)

SOAR Telescope/NSF's NOIRLab, La Serena, Chile.

Ignacio Pérez-García (I)

Instituto de Astrofísica de Andalucía (IAA-CSIC), Granada, Spain.

Classifications MeSH