Smoothed particle inference analysis and abundance calculations of DEM L71, and comparison to SN explosion models
Author:
Affiliation:
1. Department of Astronomy and AstrophysicsUniversity of Chicago Chicago Illinois
2. CIERANorthwestern University Evanston Illinois
3. Department of Astronomy and AstrophysicsPenn State University Pennsylvania
Funder
National Aeronautics and Space Administration
Publisher
Wiley
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://onlinelibrary.wiley.com/doi/pdf/10.1002/asna.202023773
Reference16 articles.
1. The Piecewise Parabolic Method (PPM) for gas-dynamical simulations
2. Smoothed Particle Inference Analysis of SNR DEM L71
3. The Physics of Supernova Blast Waves. I. Kinematics of DEM L71 in the Large Magellanic Cloud
4. High resolution spectroscopy and emission line imaging of DEM L 71 withXMM-Newton
5. Iron-rich Ejecta in the Supernova Remnant DEM L71
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1. Büyük Macellan Bulutsusundaki Süpernova Kalıntısı DEM L71'in X-ışın Özellikleri;Turkish Journal of Astronomy and Astrophysics;2023-12-31
2. Spatially Resolved Chandra Spectroscopy of Supernova Remnant DEM L71 in the Large Magellanic Cloud;Monthly Notices of the Royal Astronomical Society;2022-02-10
3. Can the Fe K-alpha Line Reliably Predict Supernova Remnant Progenitors?;The Astrophysical Journal;2021-11-01
4. Analysis of XMM-Newton Observations of Supernova Remnant W49B and Clues to the Progenitor;The Astrophysical Journal;2020-12-03
5. Elemental Abundances in Supernova Remnant W49B as Clues to Its Progenitor;Research Notes of the AAS;2020-08-05
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