Dynamical ejecta from neutron star mergers reproduce key spectral properties of AT2017gfo in polar views, with features from Sr II, La III and other ions appearing at earlier times than observed.
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GRMHD simulations of GRB 090510 predict energetics and jet opening angles consistent with observations within 1 sigma when jet angles evolve with redshift, while dynamical ejecta influence collimation and a suite of models explores broader GRB properties.
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Exploring the diversity of kilonovae with 3D radiative transfer I. The polar direction
Dynamical ejecta from neutron star mergers reproduce key spectral properties of AT2017gfo in polar views, with features from Sr II, La III and other ions appearing at earlier times than observed.
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Exploring Jet Structure and Dynamics in Short Gamma Ray Bursts: A Case Study on GRB 090510
GRMHD simulations of GRB 090510 predict energetics and jet opening angles consistent with observations within 1 sigma when jet angles evolve with redshift, while dynamical ejecta influence collimation and a suite of models explores broader GRB properties.