Results 11 to 20 of about 70,034 (292)

Comprehensive nucleosynthesis analysis for ejecta of compact binary mergers [PDF]

open access: yes, 2014
We present a comprehensive study of r-process element nucleosynthesis in the ejecta of compact binary mergers (CBMs) and their relic black-hole (BH)-torus systems.
O. Just   +10 more
semanticscholar   +3 more sources

The Osmium Isotope Signature of Phanerozoic Large Igneous Provinces

open access: yesGeophysical Monograph Series, Page 229-246., 2021

Exploring the links between Large Igneous Provinces and dramatic environmental impact

An emerging consensus suggests that Large Igneous Provinces (LIPs) and Silicic LIPs (SLIPs) are a significant driver of dramatic global environmental and biological changes, including mass extinctions.
Alexander J. Dickson   +2 more
wiley  

+2 more sources

Mapping dynamical ejecta and disk masses from numerical relativity simulations of neutron star mergers [PDF]

open access: yesClassical and quantum gravity, 2020
We present fitting formulae for the dynamical ejecta properties and remnant disk masses from the largest to date sample of numerical relativity simulations.
V. Nedora   +8 more
semanticscholar   +1 more source

Groove formation on Phobos from reimpacting orbital ejecta of the Stickney crater

open access: yesEarth and Planetary Physics, 2022
Numerous linear grooves have long been recognized as covering the surface of Phobos, but the mechanisms of their formation are still unclear. One possible mechanism is related to the largest crater on Phobos, the Stickney crater, whose impact ejecta may ...
XiangYu Xi, Min Ding, MengHua Zhu
doaj   +1 more source

Nepheline-kalsilite microperthites in ejecta from the Alban Hills (Italy) [PDF]

open access: yesBulletin of the Geological Society of Finland, 1985
Microprobe analyses carried out on exsolved nepheline and kalsilite phases of microperthites occurring in three ejecta from the Alban Hills (Roman comagmatic region) have shown: (1) a practically continuous compositional variation from Ks to Ne (bulk ...
C. Aurisicchio, M. Federico
doaj   +1 more source

The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. III. Optical and UV Spectra of a Blue Kilonova from Fast Polar Ejecta [PDF]

open access: yes, 2017
We present optical and ultraviolet spectra of the first electromagnetic counterpart to a gravitational-wave (GW) source, the binary neutron star merger GW170817.
M. Nicholl   +39 more
semanticscholar   +1 more source

A Low-mass Binary Neutron Star: Long-term Ejecta Evolution and Kilonovae with Weak Blue Emission [PDF]

open access: yesAstrophysical Journal, 2020
We study the long-term evolution of ejecta formed in a binary neutron star (NS) merger that results in a long-lived remnant NS by performing a hydrodynamics simulation with the outflow data of a numerical relativity simulation as the initial condition ...
K. Kawaguchi   +4 more
semanticscholar   +1 more source

Constraint on the Ejecta Mass for Black Hole–Neutron Star Merger Event Candidate S190814bv [PDF]

open access: yesAstrophysical Journal, 2020
We derive the upper limit to the ejecta mass of S190814bv, a black hole–neutron star (BH–NS) merger candidate, through radiative transfer simulations for kilonovae with realistic ejecta density profiles, as well as detailed opacity and heating rate ...
K. Kawaguchi, M. Shibata, Masaomi Tanaka
semanticscholar   +1 more source

A Magnetar Origin for the Kilonova Ejecta in GW170817 [PDF]

open access: yes, 2018
The neutron star (NS) merger GW170817 was followed over several days by optical-wavelength (“blue”) kilonova (KN) emission likely powered by the radioactive decay of light r-process nuclei synthesized by ejecta with a low neutron abundance (electron ...
B. Metzger, T. Thompson, E. Quataert
semanticscholar   +1 more source

Production of Very Light Elements and Strontium in the Early Ejecta of Neutron Star Mergers [PDF]

open access: yesAstrophysical Journal, 2020
We study the production of very light elements (Z < 20) in the dynamical and spiral-wave wind ejecta of binary neutron star mergers by combining detailed nucleosynthesis calculations with the outcome of numerical relativity merger simulations.
A. Perego   +12 more
semanticscholar   +1 more source

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