Article
Article
- Astronomy & Space Science
- Astronomical instruments
- ROSAT mission
- Astronomy & Space Science
- Astrophysics
- ROSAT mission
DISCLAIMER: This article is being kept online for historical purposes. Though accurate at last review, it is no longer being updated. The page may contain broken links or outdated information.
ROSAT mission
Article By:
Trümper, Joachim Max-Planck-Institut Für Extraterrestrische Physik, Garching, Germany.
Last reviewed:2001
DOI:https://doi.org/10.1036/1097-8542.YB001550
- ROSAT mission
- Moon
- Comets
- Stars
- Nuclear-burning white dwarfs
- Supernova remnants
- Neutron stars
- Galaxies and active galactic nuclei
- Clusters of galaxies
- Prospects
- Additional Reading
In recent decades the scope of observational astronomy has extended over the entire electromagnetic spectrum, and now ranges from radio waves to high-energy photons with teraelectronvolt (1 TeV = 1012 eV) energies. The different bands reveal different aspects of the universe. In the x-ray domain, at photon energies between 0.1 and 500 keV, thermal radiation from high-temperature plasmas or nonthermal radiation produced by relativistic electrons interacting with magnetic fields (synchrotron radiation) or intense photon fields (the inverse Compton effect) is observed.
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