High-velocity emission in young supernova remnants: SN 1006 and SN 1572

• 1 April 1987
• journal article
• Published by American Astronomical Society in The Astrophysical Journal
• Vol. 315, L135-L139
• https://doi.org/10.1086/184875

Abstract

Keywords

• MATHEMATICAL MODEL
• PHYSICAL PROPERTIES
• H ALPHA LINE
• SHOCK WAVES
• SHOCK WAVE
• BALMER SERIES
• SPECTRAL RESOLUTION
• KINEMATICS
• QUANTUM MECHANICS
• VARIABLE STARS
• SUPERNOVAE