Gravitational-wave detections are enabling measurements of the rate of coalescences of
binaries composed of two compact objects—neutron stars and/or black holes. The …

The production of about half of the heavy elements found in nature is assigned to a specific
astrophysical nucleosynthesis process: the rapid neutron-capture process (r process) …

To reach a deeper understanding of the origin of elements in the periodic table, we construct
Galactic chemical evolution (GCE) models for all stable elements from C (A= 12) to U (A …

The cosmic origin of elements heavier than iron has long been uncertain. Theoretical
modelling,,,,,, shows that the matter that is expelled in the violent merger of two neutron stars …

What is the origin of the oxygen we breathe, the hydrogen and oxygen (in form of water
H2O) in rivers and oceans, the carbon in all organic compounds, the silicon in electronic …

The distribution of elements in galaxies provides a wealth of information about their
production sites and their subsequent mixing into the interstellar medium. Here we …

We present UV, optical, and near-infrared (NIR) photometry of the first electromagnetic
counterpart to a gravitational wave source from Advanced Laser Interferometer Gravitational …

We present a systematic numerical relativity study of the mass ejection and the associated
electromagnetic transients and nucleosynthesis from binary neutron star (NS) mergers. We …

Constraining the Maximum Mass of Neutron Stars from Multi-messenger Observations of
GW170817 - IOPscience This site uses cookies. By continuing to use this site you agree to our …

We present the first effort to aggregate, homogenize, and uniformly model the combined
ultraviolet, optical, and near-infrared data set for the electromagnetic counterpart of the …