Search Results - "Patnaude, Daniel J."
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The Forward and Reverse Shock Dynamics of Cassiopeia A
Published in The Astrophysical journal (01-04-2022)“…Abstract We report on proper motion measurements of the forward- and reverse shock regions of the supernova remnant Cassiopeia A (Cas A), including…”
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Cooling neutron star in the Cassiopeia A supernova remnant: evidence for superfluidity in the core
Published in Monthly notices of the Royal Astronomical Society. Letters (01-03-2011)“…ABSTRACT According to recent results of Ho & Heinke, the Cassiopeia A supernova remnant contains a young (≈330‐yr‐old) neutron star (NS) which has carbon…”
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Late-time Circumstellar Interaction of SN 2017eaw in NGC 6946
Published in The Astrophysical journal (01-09-2020)“…SN 2017eaw, the tenth supernova observed in NGC 6946, was a normal Type II-P supernova with an estimated 11-13 M red supergiant progenitor. Here we present…”
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Efficient Cosmic Ray Acceleration, Hydrodynamics, and Self-Consistent Thermal X-Ray Emission Applied to Supernova Remnant RX J1713.7–3946
Published in The Astrophysical journal (20-03-2010)“…We model the broadband emission from supernova remnant (SNR) RX J1713.7-3946 including, for the first time, a consistent calculation of thermal X-ray emission…”
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Hubble Space Telescope Proper Motion Measurements of Supernova Remnant N132D: Center of Expansion and Age
Published in The Astrophysical journal (01-05-2023)“…Abstract We present proper motion measurements of the oxygen-rich ejecta of the LMC supernova remnant N132D using two epochs of Hubble Space Telescope Advanced…”
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Three-dimensional Kinematic Reconstruction of the Optically Emitting, High-velocity, Oxygen-rich Ejecta of Supernova Remnant N132D
Published in The Astrophysical journal (01-05-2020)“…We present a three-dimensional kinematic reconstruction of the optically emitting, oxygen-rich ejecta of supernova remnant N132D in the Large Magellanic Cloud…”
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Detection of the Red Supergiant Wind from the Progenitor of Cassiopeia A
Published in The Astrophysical journal (10-03-2020)“…Cassiopeia A (Cas A) is one of the best studied young Galactic supernova remnants. While it provides a rare opportunity to study in detail the remnant of a…”
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SECOND EPOCH HUBBLE SPACE TELESCOPE OBSERVATIONS OF KEPLER’S SUPERNOVA REMNANT: THE PROPER MOTIONS OF BALMER FILAMENTS
Published in The Astrophysical journal (20-01-2016)“…ABSTRACT We report on the proper motions of Balmer-dominated filaments in Kepler’s supernova remnant using high resolution images obtained with the Hubble…”
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The Center of Expansion and Age of the Oxygen-rich Supernova Remnant 1E 0102.2-7219
Published in The Astrophysical journal (01-05-2021)“…Abstract We present new proper-motion measurements of optically emitting oxygen-rich knots of supernova remnant 1E 0102.2-7219 (E0102), which are used to…”
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The Expansion of the Forward Shock of 1E 0102.2-7219 in X-Rays
Published in The Astrophysical journal (20-03-2019)“…We measure the expansion of the forward shock of the Small Magellanic Cloud supernova remnant 1E 0102.2-7219 in X-rays using Chandra X-Ray Observatory on-axis…”
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iPTF15eqv: Multiwavelength Exposé of a Peculiar Calcium-rich Transient
Published in The Astrophysical journal (01-09-2017)“…The progenitor systems of the class of "Ca-rich transients" is a key open issue in time domain astrophysics. These intriguing objects exhibit unusually strong…”
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NEW EVIDENCE FOR EFFICIENT COLLISIONLESS HEATING OF ELECTRONS AT THE REVERSE SHOCK OF A YOUNG SUPERNOVA REMNANT
Published in The Astrophysical journal (10-01-2014)“…Although collisionless shocks ar ubiquitous in astrophysics, certain key aspects of them are not well understood. In particular, the process known as…”
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The Impact of Progenitor Mass Loss on the Dynamical and Spectral Evolution of Supernova Remnants
Published in The Astrophysical journal (10-11-2017)“…There is now substantial evidence that the progenitors of some core-collapse supernovae undergo enhanced or extreme mass loss prior to explosion. The imprint…”
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Chandrasekhar and Sub-Chandrasekhar Models for the X-Ray Emission of Type Ia Supernova Remnants. I. Bulk Properties
Published in The Astrophysical journal (01-10-2018)“…Type Ia supernovae originate from the explosion of carbon-oxygen white dwarfs in binary systems, but the exact nature of their progenitors remains elusive. The…”
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The Role of Diffusive Shock Acceleration on Nonequilibrium Ionization in Supernova Remnants
Published in The Astrophysical journal (10-05-2009)“…We present results of semianalytic calculations which show clear evidence for changes in the nonequilibrium ionization behind a supernova remnant forward shock…”
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The Proper Motion of the Pulsar J1124–5916 in the Galactic Supernova Remnant G292.0+1.8
Published in The Astrophysical journal (01-06-2022)“…Abstract We present the first direct measurement of the proper motion of pulsar J1124–5916 in the young, oxygen-rich supernova remnant G292.0+1.8. Using deep…”
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A COMPARISON OF X-RAY AND OPTICAL EMISSION IN CASSIOPEIA A
Published in The Astrophysical journal (10-07-2014)“…We find weak spatial correlations between the remnant's X-ray and optical emission features on large scales, but several cases of good optical/X-ray…”
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THE ORIGIN OF KEPLER'S SUPERNOVA REMNANT
Published in The Astrophysical journal (01-09-2012)“…It is now well established that Kepler's supernova remnant (SNR) is the result of a Type Ia explosion. With an age of 407 yr and an angular diameter of ~4',…”
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MODELING BRIGHT γ-RAY AND RADIO EMISSION AT FAST CLOUD SHOCKS
Published in The Astrophysical journal (10-06-2015)“…ABSTRACT Recent observations by the Large Area Telescope on board the Fermi satellite have revealed bright γ-ray emission from middle-aged supernova remnants…”
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