Cool Stars, Stellar Systems, and the Sun pp 94-96 | Cite as
Progress report: Precise measurements of radial velocities of far-ultraviolet emission lines in stars of late spectral type
Session I: Dynamos and Stellar Activity: Observations
First Online:
Abstract
Recent high-dispersion, far-ultraviolet IUE spectra of the G-type supergiant β Draconis contain evidence for organized, persistent downflows of gas, apparently confined to a high-density component of the stellar transition zone.
Keywords
Radial Velocity Stellar Photosphere Colorado Boulder Echelle Spectrum Heliocentric Radial Velocity
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.
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References
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© Springer-Verlag 1986