A DIRECT MEASUREMENT OF THE FORWARD SHOCK SPEED IN SUPERNOVA REMNANT 0509–67.5: CONSTRAINTS ON THE AGE, AMBIENT DENSITY, SHOCK COMPRESSION FACTOR, AND ELECTRON–ION TEMPERATURE EQUILIBRATION
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/809/i=2/a=119/pdf
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1. Astrometry with the MACHO Data Archive. I. High Proper Motion Stars toward the Galactic Bulge and Magellanic Clouds
2. The Persistence of Memory, or How the X‐Ray Spectrum of SNR 0509−67.5 Reveals the Brightness of Its Parent Type Ia Supernova
3. The acceleration of cosmic rays in shock fronts - I
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2. An X-Ray Proper-motion Study of the Large Magellanic Cloud Supernova Remnant 0509-67.5;The Astronomical Journal;2022-11-02
3. A Hydro-based MCMC Analysis of SNR 0509−67.5: Revealing the Explosion Properties from Fluid Discontinuities Alone;The Astrophysical Journal;2022-10-01
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