How would a nearby kilonova look on camera?
arXiv:1905.01594 · doi:10.1119/10.0001193
Abstract
Kilonovae are cosmic optical flashes produced in the aftermath of the merger of two neutron stars. While the typical radiant flux of a kilonova can be as high as \,W, they typically occur at cosmological distances, requiring meter-class or larger telescopes for their observation. Here we explore how a kilonova would look like from Earth if it occurred in the Solar System's backyard, 1000 light years from Earth. This is a small distance on cosmological scales, with only one neutron-star merger expected to occur this close every 100,000,000 years. While humans will likely only see kilonovae at much greater distances, showing how such a nearby event would look on camera can help visualize these events, and demonstrate their unique spectral evolution.
arXiv comment6 pages, 9 figures
References in corpus (11)
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- Multi-messenger Observations of a Binary Neutron Star Merger
- Transient Events from Neutron Star Mergers
- Electromagnetic Counterparts of Compact Object Mergers Powered by the Radioactive Decay of R-process Nuclei
- A "kilonova" associated with short-duration gamma-ray burst 130603B
- Effect of a High Opacity on the Light Curves of Radioactively Powered Transients from Compact Object Mergers
- Mergers of neutron star black hole binaries with small mass ratios: nucleosynthesis, gamma-ray bursts and electromagnetic transients
- Circular polarization in the optical afterglow of GRB 121024A
- Modeling Supernova-like Explosions Associated with Gamma-ray Bursts with Short Durations
- Interactive Visualization and Simulation of Astronomical Nebulae
- Estimating the Fuel Supply Rate on the Galactic Disk from High Velocity Clouds (HVCs) Infall