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X-ray spectroscopic observations and modeling of supernova remnants
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Shull, J. M. |
| Copyright Year | 1981 |
| Description | The X-ray observations of young remnants and their theoretical interpretation are described. A number of questions concerning the nature of the blast wave interaction with the interstellar gas and grains and of atomic processes in these hot plasmas are considered. It is concluded that future X-ray spectrometers with high collecting area, moderate spectral resolution and good spatial resolution can make important contributions to the understanding of supernova remnants in the Milky Way and neighboring galaxies and of their role in the global chemical and dynamical evolution of the interstellar medium. |
| File Size | 454932 |
| Page Count | 11 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19820018183 |
| Archival Resource Key | ark:/13960/t2v45jg3q |
| Language | English |
| Publisher Date | 1981-11-01 |
| Access Restriction | Open |
| Subject Keyword | Astronomy Stellar Spectra Supernova Remnants Neutron Stars Stellar Mass Ejection Plasmas Physics X Ray Spectroscopy Spectrometers Spectroscopic Analysis Abundance X Ray Spectra X Ray Astronomy Black Holes Astronomy Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |
