Abstract
We argue that the majority of radio supernova remnants have a three-dimensional distribution of emissivity which is barrel shaped, with little emission from the end-caps. We examine some mechanisms which could produce this distribution.
Register to see more suggestions
Mendeley helps you to discover research relevant for your work.
Already have an account? Sign in
Sign up for freeCite
CITATION STYLE
APA
Kesteven, M. J., & Caswell, J. L. (1988). Barrel-Shaped Supernova Remnants. International Astronomical Union Colloquium, 101, 359–361. https://doi.org/10.1017/s0252921100102660
Readers over time
Readers' Seniority
Readers' Discipline
