Results 101 to 110 of about 12,699 (236)
Multiband Emission from Star–Disk Collisions and Implications for Quasiperiodic Eruptions
We perform two-dimensional, multigroup radiation hydrodynamic simulations to explore the observational properties of a solar-like star colliding with an accretion disk around a supermassive black hole at a separation of ∼100 gravitational radii.
Xiaoshan Huang +2 more
doaj +1 more source
Styles of ejecta emplacement under atmospheric conditions
Laboratory experiments provide essential first-order constraints on processes affecting ballistic ejecta and styles of ejecta emplacement under different atmospheric environments at planetary scales.
Schultz, P. H.
core
The formation of fluidized ejecta on Mars by granular flows
From the proceedings of the Workshop on the Role of Volatiles and Atmospheres on Martian Impact Craters held on July 11-14, 2005, at the Johns Hopkins University Applied Physics Laboratory.A simple granular flow model is used to investigate some of the ...
Barnouin-Jha, Olivier S., Wada, Koji
core +1 more source
A precambrian proximal ejecta blanket from Scotland
Ejecta blankets around impact craters are rarely preserved on Earth. Although impact craters are ubiquitous on solid bodies throughout the solar system, on Earth they are rapidly effaced, and few records exist of the processes that occur during ...
Hesselbo, Stephen +9 more
core +1 more source
Orbital Capture of Ejecta into Periodic Orbits around Binary Asteroid (65803) Didymos
The successful impact of the Double Asteroid Redirection Test (DART) spacecraft on Dimorphos enabled the first-ever extensive observation of a postimpact ejecta tail from a binary asteroid system.
Xiaoyu Fu +28 more
doaj +1 more source
SN1987A at 18 Years: Ejecta-Ring Interaction
International audienceAfter 18 years the outer parts of the ejecta of SN1987A are interacting with the inner ring. This ejecta-ring interaction is the source of most of the activity associated with the supernova.
de Buizer, I. James M. +8 more
core +1 more source
Type Iax Supernovae as a Source of Iron-rich Silicate Dust
We model the formation of dust in the ejecta of Type Iax supernovae (SNe), which is a low-luminosity subclass of Type Ia SNe. A nonequilibrium chemical kinetic approach is adopted to trace the synthesis of molecules, molecular clusters, and dust grains ...
Aman Kumar, Arkaprabha Sarangi
doaj +1 more source
Simulated 3D 56Ni Distributions of Type IIp Supernovae
We present the first three-dimensional study of the asymptotic ejecta distributions for a suite of theoretical Type IIp supernovae originating from red supergiant (RSG) progenitors.
David Vartanyan +6 more
doaj +1 more source
We present 1800 multiwavelength Type Ib/c supernovae light-curve models obtained by running the radiation transport code Sedona and varying the mass distribution, velocity profile, and abundance ejecta profiles of helium star progenitors.
S. Karthik Yadavalli +5 more
doaj +1 more source
Fast dynamic ejecta in neutron star mergers
The ejection of neutron-rich matter is one of the most important consequences of a neutron star merger. While the bulk of the matter is ejected at fast, but non-relativistic velocities (similar to 0.2c), a small amount of mildly relativistic dynamic ...
Diener, Peter +7 more
core +1 more source

