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The velocity and composition of supernova ejecta
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Colgate, S. A. |
| Copyright Year | 1971 |
| Description | In case of the Gum nebula, a pulsar - a presumed neutron star - is believed to be a relic of the supernova explosion. Regardless of the mechanism of the explosion, the velocity distribution and composition of the ejected matter will be roughly the same. The reimploding mass fraction is presumed to be neutron rich. The final composition is thought to be roughly 1/3 iron and 2/3 silicon, with many small fractions of elements from helium to iron. The termination of helium shell burning occurs because the shell is expanded and cooled by radiation stress. The mass fraction of the helium burning shell was calculated. |
| File Size | 269747 |
| Page Count | 7 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19720004110 |
| Archival Resource Key | ark:/13960/t8gf5jx4c |
| Language | English |
| Publisher Date | 1971-09-01 |
| Access Restriction | Open |
| Subject Keyword | Space Sciences Conferences Supernovae Pulsars Chemical Composition Velocity Distribution Helium Nebulae Interstellar Matter Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |