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Stellar x-ray temporal variations
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Holt, S. S. |
| Copyright Year | 1972 |
| Description | Two separate theoretical models of X-ray sources were proposed, based on the premise that a pulsar can be hidden underneath a thick plasma cloud. The X-ray emission would come secondarily from the pulsar energy from the cloud underneath. Upper limits to the pulsed fraction for those conditions causing the most difficult detection of fluctuations are shown, along with power density and source of power spectra. |
| File Size | 150946 |
| Page Count | 5 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19720026165 |
| Archival Resource Key | ark:/13960/t3mw76c7m |
| Language | English |
| Publisher Date | 1972-06-01 |
| Access Restriction | Open |
| Subject Keyword | Space Radiation X Rays Theoretical Physics Radiation Sources Astronomical Models Pulsars Ntrs Nasa Technical Reports ServerĀ (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Technical Report |