Infrared Ejecta and Cold Dust in the Young Supernova Remnant N132D [PDF]
We present Spitzer, Wide-field Infrared Survey Explorer (WISE), and Herschel observations of the young supernova remnant (SNR) N132D in the Large Magellanic Cloud, including 3–40 μ m Spitzer Infrared Spectrograph (IRS) mapping, 12 μ m WISE and 70, 100 ...
Jeonghee Rho+3 more
doaj +2 more sources
Impact Ejecta near the Impact Point Observed using Ultra-high-speed Imaging and SPH Simulations, and a Comparison of the Two Methods [PDF]
High-speed impact ejecta at velocities comparable to the impact velocity are expected to contribute to material transport between planetary bodies and deposition of ejecta far from the impact crater.
Genda, Hidenori+3 more
core +2 more sources
XMM-Newton Large Program on SN1006 - II: Thermal Emission [PDF]
Based on the XMM-Newton large program on SN1006 and our newly developed spatially resolved spectroscopy tools (Paper~I), we study the thermal emission from ISM and ejecta of SN1006 by analyzing the spectra extracted from 583 tessellated regions dominated
Bocchino, Fabrizio+4 more
core +5 more sources
GRB 060206: hints of precession of the central engine? [PDF]
Aims. The high-redshift (z=4.048) gamma-ray burst GRB 060206 showed unusual behavior, with a significant rebrightening by a factor of ~4 at about 3000 s after the burst. We argue that this rebrightening implies that the central engine became active again
Liu, X. W., Lu, T., Wu, X. F.
core +3 more sources
Hydrodynamic modelling of ejecta shrapnel in the Vela supernova remnant [PDF]
Many supernova remnants (SNRs) are characterized by a knotty ejecta structure. The Vela SNR is an excellent example of remnant in which detached clumps of ejecta are visible as X-ray emitting bullets that have been observed and studied in great detail ...
Bocchino, F.+4 more
core +3 more sources
Co-authored with artist Anthony Cervino, this book was produced on the occasion of the exhibition of the same name at CulturalDC\u27s Flashpoint Gallery in Washington, DC.
Cervino, Anthony, Egan, Shannon
core +2 more sources
Linking Analytic Light-curve Models to Physical Properties of Kilonovae [PDF]
In binary neutron star mergers, lanthanide-rich dynamical ejecta and lanthanide-poor postmerger ejecta have often been linked to red and blue kilonova emission, respectively.
Ayari Kitamura+3 more
doaj +2 more sources
Circumstellar ejecta around LBV’s [PDF]
AbstractThe properties of circumstellar shells around LBV’s are reviewed. Some LBV’s are surrounded by very extended nebulosities, similar to classical planetary nebulae, with AG Car as the prototype. The masses of these nebulae are of the order of a solar mass and their kinematic ages are about 104years.
O. Stahl
openaire +3 more sources
The Osmium Isotope Signature of Phanerozoic Large Igneous Provinces
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