Rapid Postshock Cooling and Pressure-driven Shell-phase Evolution of the Galactic Halo SNR G70.0–21.5
Author:
Funder
Chandra X-ray Center
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/1538-4357/ab5e84/pdf
Reference37 articles.
1. Interplay between physics and geometry in Balmer filaments: the case of SN 1006
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