Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982esasp.176..497h&link_type=abstract
In ESA 3rd European IUE Conf. p 497-501 (SEE N83-11889 02-88)
Astronomy and Astrophysics
Astronomy
European Space Programs, Scientific Satellites, Spaceborne Astronomy, Ultraviolet Astronomy, Binary Stars, Chromosphere, Extreme Ultraviolet Radiation, Flare Stars, Giant Stars, Main Sequence Stars, Neutron Stars, Stellar Coronas, Stellar Spectra, Supergiant Stars, White Dwarf Stars
Scientific paper
The importance of Magellan observing peculiar stellar objects, young contracting stars or far-evolved objects is discussed. Magellan could observe the EUV spectrum of white dwarfs, chromospheres and coronae of red dwarfs and especially flare stars, chromospheres and coronae of about 20 main sequence stars in the spectral range AO/K5, and could detect neutron stars and measure their continuous spectrum. In the spectral range from 913 to 1500A, it could provide data on nebular variables, flare stars, cataclysmic variables, hot subdwarfs and white dwarfs, interacting binaries, and late giants and supergiants.
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