No CrossRef data available.
Article contents
Ultraviolet Observations of 31 and 32 Cygni
Published online by Cambridge University Press: 14 August 2015
Extract
Ultraviolet observations of the Zeta Aurigae systems appear to have several advantages over comparable visual wavelength studies. A wide range of large optical depth resonance lines of abundant species permit the study of the supergiant atmosphere and circumstellar environment at virtually all phases. The International Ultraviolet Explorer satellite (Boggess, et al., 1978) is well suited to obtaining spectra between 1150 and 3200 A, although the competition for observing time is non-negligible.
- Type
- X. … and The Rest (Symbiotics, Supergiants, Planetaries, Population II Systems)
- Information
- Copyright
- Copyright © Reidel 1980