Supernova Remnant Crossing a Density Jump: A Thin‐Shell Model
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/595/i=1/a=227/pdf
Reference22 articles.
1. Aschenbach, B. 2002, in Proc. 270 WE-Heraeus Seminar on Neutron Stars, Pulsars, and Supernova Remnants, ed. W. Becker, H. Lesch, & J. Trumper (MPE Rep. 278; Garching: MPE), 13
2. Supernova Remnants Associated with Molecular Clouds in the Large Magellanic Cloud
3. High-resolution X-ray spectroscopy and imaging of supernova remnant N132D
4. Hubble Space TelescopeObservations of Oxygen‐rich Supernova Remnants in the Magellanic Clouds. II. Elemental Abundances in N132D and 1E 0102.2−7219
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1. Hubble Space Telescope Proper Motion Measurements of Supernova Remnant N132D: Center of Expansion and Age;The Astrophysical Journal;2023-05-01
2. LMC N132D: A mature supernova remnant with a power-law gamma-ray spectrum extending beyond 8 TeV;Astronomy & Astrophysics;2021-10-28
3. ALMA CO Observations of Gamma-Ray Supernova Remnant N132D in the Large Magellanic Cloud: Possible Evidence for Shocked Molecular Clouds Illuminated by Cosmic-Ray Protons;The Astrophysical Journal;2020-10-12
4. Plasma Diagnostics of the Supernova Remnant N132D using Deep XMM–Newton Observations with the Reflection Grating Spectrometer;The Astrophysical Journal;2020-08-28
5. Three-dimensional Kinematic Reconstruction of the Optically Emitting, High-velocity, Oxygen-rich Ejecta of Supernova Remnant N132D;The Astrophysical Journal;2020-05-07
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