The Emergence of a Lanthanide-rich Kilonova Following the Merger of Two Neutron Stars
University of Leicester · University of Warwick · +24 more institutions
Abstract
Abstract We report the discovery and monitoring of the near-infrared counterpart (AT2017gfo) of a binary neutron-star merger event detected as a gravitational wave source by Advanced Laser Interferometer Gravitational-wave Observatory (LIGO)/Virgo (GW170817) and as a short gamma-ray burst by Fermi Gamma-ray Burst Monitor (GBM) and Integral SPI-ACS (GRB 170817A). The evolution of the transient light is consistent with predictions for the behavior of a “kilonova/macronova” powered by the radioactive decay of massive neutron-rich nuclides created via r -process nucleosynthesis in the neutron-star ejecta. In particular, evidence for this scenario is found from broad features seen in Hubble Space Telescope infrared…
Citation impact
- FWCI
- 59.53
- Percentile
- 100%
- References
- 97
Authors
54Topics & keywords
- Kilonova
- Physics
- Nucleosynthesis
- Neutron star
- LIGO
- Astrophysics
- Ejecta
- Gravitational wave
Funding
- UDU.S. Department of EnergyAwards: DE-AC52-06NA25396, AC52-06NA25396
- VFVillum FondenAward: 16599
- USUK Space Agency
- STSpace Telescope Science Institute
- ECEuropean CommissionAward: 725246
- VVetenskapsrådetAwards: 2016-03657_3, Dnr 2016-06012, 2016-06012
- IDInstituto de Astrofísica de Canarias
- NNNational Nuclear Security AdministrationAward: DE-AC52-06NA25396
- SAScience and Technology Facilities CouncilAwards: ST/N000064/1, ST/L00061X/1, ST/N000927/1, ST/N005805/1, ST/P000495, ST/P000495/1, ST/N000757/1, ST/J001465/1, Gravitational Waves, ST/J000345/1, ST/I006285/1, ST/M000966/1, ST/P000495/1, ST/N005805/1, ST/H001972/1, ST/L000962/1, ST/N005430/1
- LALos Alamos National LaboratoryAwards: AC52-06NA25396, No. DE-AC52-06NA25396, DE-AC52-06NA25396