Katsuda, Satoru, Petre, Robert, Long, Knox S., Reynolds, Stephen P., Winkler, P. Frank, Mori, Koji, ...
We report on the first X-ray proper-motion measurements of the nonthermally-dominated forward shock in the northeastern limb of SN 1006, based on two Chandra observations taken in 2000 and 2008. We...
Ejecta, Dust, and Synchrotron Radiation in B0540-69.3: A More Crab-Like Remnant than the Crab (2008)
Williams, Brian J., Borkowski, Kazimierz J., Reynolds, Stephen P., Raymond, John C., Long, Knox S., Morse, Jon A., ...
We present near and mid-infrared observations of the pulsar-wind nebula (PWN) B0540-69.3 and its associated supernova remnant made with the {\it Spitzer Space Telescope}. We report detections of the...
X-Ray Emitting Ejecta of Supernova Remnant N132D (2007)
Borkowski, Kazimierz J., Hendrick, Sean P., Reynolds, Stephen P.
The brightest supernova remnant in the Magellanic Clouds, N132D, belongs to the rare class of oxygen-rich remnants, about a dozen objects that show optical emission from pure heavy-element ejecta....
Blair, William P., Ghavamian, Parviz, Long, Knox S., Williams, Brian J., Borkowski, Kazimierz J., Reynolds, Stephen P., ...
We present 3.6 - 160 micron infrared images of Kepler's supernova remnant (SN1604) obtained with the IRAC and MIPS instruments on the Spitzer Space Telescope. We also present MIPS SED low resolution...
Dust Destruction in Type Ia Supernova Remnants in the Large Magellanic Cloud (2006)
Borkowski, Kazimierz J., Williams, Brian J., Reynolds, Stephen P., Blair, William P., Ghavamian, Parviz, Sankrit, Ravi, ...
We present first results from an extensive survey of Magellanic Clouds supernova remnants (SNRs) with the Spitzer Space Telescope. We describe IRAC and MIPS imaging observations at 3.6, 4.5, 5.8, 8,...
Magnetohydrodynamic Models for the Structure of Pulsar-Wind Nebulae (2003)
The Crab Nebula is well-described at optical wavelengths and above by a steady-state magnetohydrodynamic model due to Kennel and Coroniti (1984). Can this class of model describe other pulsar-wind...
Near-Infrared Synchrotron Emission from Cas A (2003)
Rho, Jeonghee, Reynolds, Stephen P., Reach, William T., Jarrett, Tom H., Allen, Glenn E.
High energy observations of Cas A suggested the presence of synchrotron radiation, implying acceleration of cosmic rays by young supernova remnants. We detect synchrotron emission from Cas A in the...
X-Ray Synchrotron Emitting Fe-Rich Ejecta in SNR RCW 86 (2002)
Rho, Jeonghee, Dyer, Kristy K., Borkowski, Kazimierz J., Reynolds, Stephen P.
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 and above 2 keV...
Dyer, Kristy K., Reynolds, Stephen P., Borkowski, Kazik J., Petre, Robert
The 10^51 ergs released in a supernova have far reaching consequences in the galaxy, determining elemental abundances, accelerating cosmic rays, and affecting the makeup of the interstellar medium....
Low Frequency Insights Into Supernova Remnants (2000)
Dyer, Kristy K., Reynolds, Stephen P., Borkowski, Kazik J.
Low frequency observations at 330 and 74 MHz can provide new insights into supernova remnants (SNR). We can test theoretical predictions for spectral index variations. Nonlinear models of shock...
Baring, Matthew G., Ellison, Donald C., Reynolds, Stephen P., Grenier, Isabelle, Goret, Philippe
Supernova remnants (SNRs) are widely believed to be the principal source of galactic cosmic rays. Such energetic particles can produce gamma-rays and lower energy photons via interactions with the...
Shock Acceleration and Gamma-Ray Emitting Supernova Remnants (1997)
Baring, Matthew G., Ellison, Donald C., Reynolds, Stephen P., Grenier, Isabelle A., Goret, Philippe
Diffusive shock acceleration in the environs of a remnant's expanding shell is a popular candidate for the origin of SNR gamma-rays. In this paper, results from our study of non-linear effects in...