Search Results - "Raymond, John C."
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A Nitrogen-rich Supernova Remnant in M31: Interaction with the Circumstellar Medium at Late Times
Published in The Astrophysical journal (01-09-2023)“…Abstract We present the discovery of a supernova remnant in M31 which is unlike any other remnant known in that galaxy. An optical ground-based spectrum of…”
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The Dynamical Behavior of Reconnection-driven Termination Shocks in Solar Flares: Magnetohydrodynamic Simulations
Published in The Astrophysical journal (20-12-2018)“…In eruptive solar flares, termination shocks (TSs), formed when high-speed reconnection outflows collide with closed dense flaring loops, are believed to be…”
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3
The Distance to the S147 Supernova Remnant
Published in The Astrophysical journal (01-06-2024)“…In the absence of a parallax distance to a pulsar or a surviving binary in a supernova remnant (SNR), distances to Galactic SNRs are generally very uncertain…”
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Third Epoch HST Imaging of a Nonradiative Shock in the Cygnus Loop Supernova Remnant
Published in The Astrophysical journal (01-05-2023)“…Abstract We present new HST/WFC3 optical images of a region in the northeastern part of the Cygnus Loop supernova remnant, which includes a well-studied…”
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Nonequilibrium Ionization Modeling of Petschek-type Shocks in Reconnecting Current Sheets in Solar Eruptions
Published in The Astrophysical journal (01-02-2023)“…Abstract Nonequilibrium ionization (NEI) is essentially required for astrophysical plasma diagnostics once the plasma status departs from the assumption of…”
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Electron–Ion Temperature Ratio in Astrophysical Shocks
Published in The Astrophysical journal (01-06-2023)“…Abstract Collisionless shock waves in supernova remnants and the solar wind heat electrons less effectively than they heat ions, as is predicted by kinetic…”
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He Abundance of Dense Circumstellar Clumps in the Cassiopeia A Supernova Remnant
Published in The Astrophysical journal (01-03-2023)“…Abstract We report on the result of He abundance analysis of dense circumstellar clumps in the young supernova remnant Cassiopeia A. These clumps, which are…”
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A Massive Shell of Supernova-formed Dust in SNR G54.1+0.3
Published in The Astrophysical journal (10-02-2017)“…While theoretical models of dust condensation predict that most refractory elements produced in core-collapse supernovae (SNe) efficiently condense into dust,…”
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Three-dimensional Simulation of Thermodynamics on Confined Turbulence in a Large-scale CME-flare Current Sheet
Published in The Astrophysical journal (01-10-2023)“…Abstract Turbulence plays a key role in forming the complex geometry of the large-scale current sheet (CS) and fast energy release in a solar eruption. In this…”
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10
Observations and Interpretation of a Low Coronal Shock Wave Observed in the EUV by the SDO/AIA
Published in The Astrophysical journal (10-09-2011)“…Taking advantage of both the high temporal and spatial resolutions of the Atmospheric Imaging Assembly on board the Solar Dynamics Observatory, we studied a…”
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Solar Energetic Particle Charge States and Abundances with Nonthermal Electrons
Published in The Astrophysical journal (01-03-2024)“…Abstract An important aspect of solar energetic particle (SEP) events is their source populations. Elemental abundance enhancements of impulsive SEP events,…”
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12
The Spin of a Newborn Black Hole: Swift J1728.9-3613
Published in The Astrophysical journal (01-04-2023)“…Abstract The origin and distribution of stellar-mass black hole spins are a rare window into the progenitor stars and supernova events that create them. Swift…”
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The Cygnus Loop’s distance, properties, and environment driven morphology
Published in Monthly notices of the Royal Astronomical Society (01-12-2018)Get full text
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Turbulence and Energetic Particles in Radiative Shock Waves in the Cygnus Loop. I. Shock Properties
Published in The Astrophysical journal (01-05-2020)“…We have obtained a contiguous set of long-slit spectra of a shock wave in the Cygnus Loop to investigate its structure, which is far from the morphology…”
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Numerical Simulations of Supernova Remnant Evolution in a Cloudy Interstellar Medium
Published in The Astrophysical journal (01-09-2017)“…The mixed morphology class of supernova remnants has centrally peaked X-ray emission along with a shell-like morphology in radio emission. White & Long…”
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G107.0+9.0: a new large optically bright, radio, and X-Ray faint galactic supernova remnant in Cepheus
Published in Monthly notices of the Royal Astronomical Society (01-11-2020)“…ABSTRACT Wide-field H α images of the Galactic plane have revealed a new supernova remnant (SNR) nearly 3 deg in diameter centred at l = 107.0, b = +9.0. Deep…”
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MMT Spectroscopy of Supernova Remnant Candidates in M33
Published in The Astrophysical journal (10-03-2018)“…To date, over 220 emission nebulae in M33 have been identified as supernova remnants (SNRs) or SNR candidates, principally through [S ii]:H line ratios that…”
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18
3D MHD Time-dependent Charge State Ionization and Recombination Modeling of the Bastille Day Coronal Mass Ejection
Published in The Astrophysical journal (01-09-2023)“…Abstract Heavy ion signatures of coronal mass ejections (CMEs) indicate that rapid and strong heating takes place during the eruption and early stages of…”
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The Cygnus Loop: Shock Precursors and Electron–Ion Equilibration
Published in The Astrophysical journal (01-09-2023)“…Abstract The outermost edges of some supernova remnants are marked by filaments of pure Balmer line emission produced by nonradiative shock fronts. The H α…”
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The Peculiar Ejecta Rings in the O-Rich Supernova Remnant Puppis A: Evidence of a Binary Interaction?
Published in The Astrophysical journal (01-01-2024)“…Abstract Near the center of the Puppis A supernova remnant a series of nested, optically emitting rings of high-velocity ejecta (known as “the Swirl”) were…”
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