Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Oak Ridge National LaboratoryUS200 papers
- Los Alamos National LaboratoryUS198 papers
- Duke UniversityUS187 papers
- Triangle Universities Nuclear LaboratoryUS171 papers
- University of Tennessee at KnoxvilleUS134 papers
- University of WashingtonUS134 papers
- University of North Carolina at Chapel HillUS130 papers
- Lawrence Berkeley National LaboratoryUS119 papers
- University of California, BerkeleyUS103 papers
- Centre National de la Recherche ScientifiqueFR98 papers
- Indiana University BloomingtonUS94 papers
- Massachusetts Institute of TechnologyUS93 papers
7 papers · 2 filters
Stability of Standing Accretion Shocks, With an Eye Toward Core Collapse Supernovae
John M. Blondin, Anthony Mezzacappa, Christine DeMarino
We examine the stability of standing, spherical accretion shocks. Accretion shocks arise in core collapse supernovae (the focus of this paper), star formation, and accreting white…
BBN And CMB Constraints On Dark Energy
James P. Kneller, Gary Steigman
Current observational data favor cosmological models which differ from the standard model due to the presence of some form of dark energy and, perhaps, by additional contributions…
X-Ray Synchrotron Emitting Fe-Rich Ejecta in SNR RCW 86
Jeonghee Rho, Kristy K. Dyer, Kazimierz J. Borkowski +1
Supernova remnants may exhibit both thermal and nonthermal X-ray emission. We present Chandra observations of RCW 86. Striking differences in the morphology of X-rays below 1 keV a…
Delayed Nickel Decay in Gamma Ray Bursts
G. C. McLaughlin, R. A. M. J. Wijers
Recently observed emission lines in the X-ray afterglow of gamma ray bursts suggest that iron group elements are either produced in the gamma ray burst, or are present nearby. If t…
Off-Axis Neutrino Scattering in GRB Central Engines
Nathan D. George, Arkady Kheyfets, John M. McGhee +1
The search for an understanding of an energy source great enough to explain the gamma-ray burst (GRB) phenomena has attracted much attention from the astrophysical community since…
The Angular Expansion and Distance of the Planetary Nebula BD+30 3639
Jianyang Li, J. Patrick Harrington, Kazimierz J. Borkowski
The WFPC2 camera aboard the HST was used to obtain images of the planetary nebula BD+30 3639 at two epochs separated by 5.663 years. The expansion of the nebula in the H-alpha and…
Nonlinear Particle Acceleration in Relativistic Shocks
Donald C. Ellison, Glen P. Double
Monte Carlo techniques are used to model nonlinear particle acceleration in parallel collisionless shocks of various speeds, including mildly relativistic ones. When the accelerati…