Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988esasp.281b..45r&link_type=abstract
In ESA, Proceedings of the Celebratory Symposium on a Decade of UV Astronomy with the IUE Satellite, Volume 2 p 45-51 (SEE N89-1
Astronomy and Astrophysics
Astronomy
2
Doppler Effect, Imaging Techniques, Iue, Spaceborne Astronomy, Stellar Activity, Ultraviolet Astronomy, Ultraviolet Spectra, Cool Stars, Stellar Atmospheres, Stellar Rotation
Scientific paper
High-dispersion IUE spectra were used to study the geometrical and physical characteristics of discrete structures in the outer atmospheres of rapidly-rotating active stars. As these stars rotate, such structures move across the stellar disk with a changing radial velocity producing narrow Doppler-shifted line components, which migrate across the rotationally broadened line profiles emitted by the immaculate star. By decomposing the observed emission line profiles into their individual components, it is possible to locate the discrete features on the stellar surface and to derive their physical characteristics. The spectral, or Doppler, imaging techniques are used to derive crude bi- or tridimensional images of stellar atmospheres and to study pure flare and plage emissions by spectral decomposition of high-resolution line profiles. Results are consistent with evidence collected at other wavelengths and using independent techniques. Therefore, it is promising to pursue this method, even though it requires data to be obtained over many time scales and over many orbits, in order to disentangle stable features from transient phenomena.
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