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Euve spectroscopy of the accretion region in am herculis
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Paerels, Frederik |
| Copyright Year | 1997 |
| Description | Progress in determining the gravitational energy conversion balance in accreting white dwarf stars is reported. Detailed photospheric spectra of the white dwarf stars in the brightest magnetic cataclysmic binaries, in the region where most of the energy is radiated by the stellar atmosphere - in the extreme ultraviolet band is obtained. |
| File Size | 203342 |
| Page Count | 4 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19970040692 |
| Archival Resource Key | ark:/13960/t1vf1rw9s |
| Language | English |
| Publisher Date | 1997-01-01 |
| Access Restriction | Open |
| Subject Keyword | Astronomy Stellar Spectra Fourier Transformation White Dwarf Stars Extreme Ultraviolet Explorer Satellite Spectroscopic Analysis Accretion Disks Photosphere Stellar Atmospheres Cataclysmic Variables X Rays Emission Spectra Energy Conversion Gravitational Binding Energy Line Spectra Extreme Ultraviolet Radiation 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 |