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
8 papers · 2 filters
Hubble Space Telescope WFPC-2 Imaging of Cassiopeia A
Robert A. Fesen, Jon A. Morse, Roger A. Chevalier +4
The young SNR Cassiopeia A was imaged with WFPC-2 through four filters selected to capture the complete velocity range of the remnant's main shell in several important emission lin…
Pulsar Wind Nebulae in Evolved Supernova Remnants
John M. Blondin, Roger A. Chevalier, Dargan M. Frierson
For pulsars similar to the one in the Crab Nebula, most of the energy input to the surrounding wind nebula occurs on a timescale of less than 1000 years; during this time, the nebu…
Tests of Galactic Cosmic Ray Source Models
L O'C Drury, D C Ellison, F A Aharonian +9
This report discusses the possibilities for observational tests of current models and ideas regarding the origin of the Galactic Cosmic Rays using facilities which are already avai…
Broad-band Observations and Modeling of the Shell-Type Supernova Remnant G347.3-0.5
Donald C. Ellison, Patrick Slane, Bryan M. Gaensler
The supernova remnant G347.3--0.5 emits a featureless power-law in X-rays, thought to indicate shock-acceleration of electrons to high energies. We here produce a broad-band spectr…
Spatially-resolved Thermal Continuum Absorption against the Supernova Remnant W49B
C. K. Lacey, T. Joseph W. Lazio, Namir E. Kassim +3
We present sub-arcminute resolution imaging of the Galactic supernova remnant W49B at 74 MHz (25") and 327 MHz (6"), the former being the lowest frequency at which the source has b…
Rayleigh-Taylor Instabilities in Young Supernova Remnants Undergoing Efficient Particle Acceleration
John M. Blondin, Donald C. Ellison
We employ hydrodynamic simulations to study the effects of high shock compression ratios, as expected for fast shocks with efficient particle acceleration, on the convective instab…
Australia Telescope Compact Array Observations of the OH Star Roberts 22: Resolved Images of OH Emission
Kristy Dyer, W. Miller Goss, Athol Kemball
We have imaged the unusual OH/IR object G 284-0.8 (Roberts 22) in the OH transitions at 1612, 1665 and 1667 MHz using the Australia Telescope Compact Array in Narrabri, NSW, Austra…
Spatially Varying X-ray Synchrotron Emission in SN 1006
Kristy Dyer, Stephen Reynolds, Kazik Borkowski +1
A growing number of both galactic and extragalactic supernova remnants show non-thermal (non-plerionic) emission in the X-ray band. New synchrotron models, realized as SRESC and SR…