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Cited article:

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The Astrophysical Journal 914 (2) 103 (2021)
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RGS Observations of Ejecta Knots in Tycho’s Supernova Remnant

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Excluding supersoft X-ray sources as progenitors for four Type Ia supernovae in the Large Magellanic Cloud

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KEPLER’SSUPERNOVA: AN OVERLUMINOUS TYPE Ia EVENT INTERACTING WITH A MASSIVE CIRCUMSTELLAR MEDIUM AT A VERY LATE PHASE

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Oxygen emission in remnants of thermonuclear supernovae as a probe for their progenitor system

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Monthly Notices of the Royal Astronomical Society 449 (2) 1441 (2015)
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Radio-continuum study of Large Magellanic Cloud supernova remnant J0509−6731

L. M. Bozzetto, M. D. Filipović, D. Urošević, R. Kothes and E. J. Crawford
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Parametric studies of cosmic ray acceleration in supernova remnants

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INVERSE COMPTON X-RAY EMISSION FROM SUPERNOVAE WITH COMPACT PROGENITORS: APPLICATION TO SN2011fe

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New insights into SNR evolution revealed by the discovery of recombining plasmas

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DUSTY BLAST WAVES OF TWO YOUNG LARGE MAGELLANIC CLOUD SUPERNOVA REMNANTS: CONSTRAINTS ON POST-SHOCK COMPRESSION

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TEMPERATURE EQUILIBRATION BEHIND THE SHOCK FRONT: AN OPTICAL AND X-RAY STUDY OF RCW 86

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EXPANSION VELOCITY OF EJECTA IN TYCHO's SUPERNOVA REMNANT MEASURED BY DOPPLER BROADENED X-RAY LINE EMISSION

Asami Hayato, Hiroya Yamaguchi, Toru Tamagawa, et al.
The Astrophysical Journal 725 (1) 894 (2010)
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COSMIC-RAY ACCELERATION EFFICIENCY VERSUS TEMPERATURE EQUILIBRATION: THE CASE OF SNR 0509-67.5

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