Patrick Slane
0000-0002-6986-6756
21 papers found
Refreshing results…
Dust Destruction in Nonradiative Shocks
Probing the Innermost Ejecta Layers in Supernova Remnant Kes 75: Implications for the Supernova Progenitor
Chandrasekhar and Sub-Chandrasekhar Models for the X-Ray Emission of Type Ia Supernova Remnants. I. Bulk Properties
Investigating the Structure of Vela X
J0453-6655, the Supernova Remnant in N4D
The Impact of Progenitor Mass Loss on the Dynamical and Spectral Evolution of Supernova Remnants
Numerical Simulations of Supernova Remnant Evolution in a Cloudy Interstellar Medium
Evolution of a Pulsar Wind Nebula within a Composite Supernova Remnant
A Massive Shell of Supernova-formed Dust in SNR G54.1+0.3
Deepchandraobservations of the Pulsar Wind Nebula Created by Psr B0355+54
Probing X-Ray Absorption and Optical Extinction in the Interstellar Medium Usingchandraobservations of Supernova Remnants
Radio Polarization Observations of the Snail: A Crushed Pulsar Wind Nebula in G327.1–1.1 With a Highly Ordered Magnetic Field
Late-Time Evolution of Composite Supernova Remnants: Deepchandraobservations and Hydrodynamical Modeling of a Crushed Pulsar Wind Nebula in Snr G327.1-1.1
The Properties of the Progenitor Supernova, Pulsar Wind, and Neutron Star Inside Pwn G54.1+0.3
MODELING BRIGHTγ-RAY AND RADIO EMISSION AT FAST CLOUD SHOCKS
X-Ray Analysis of the Proper Motion and Pulsar Wind Nebula for Psr J1741-2054
ERRATUM: “A CR-HYDRO-NEI MODEL OF THE STRUCTURE AND BROADBAND EMISSION FROMTYCHO'S SUPERNOVA REMNANT” (2014, ApJ, 783, 33)
Asymmetry in the Observed Metal-Rich Ejecta of the Galactic Type Ia Supernova Remnant G299.2–2.9
X-Ray Observation of the Shocked Red Supergiant Wind of Cassiopeia A
Identification of a Jet-Driven Supernova Remnant in the Small Magellanic Cloud: Possible Evidence for the Enhancement of Bipolar Explosions at Low Metallicity
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