Ultraviolet spectroscopy of F and G supergiants with IUE. I - First results of Cepheid variables

Details Ultraviolet spectroscopy of F and G supergiants with IUE. I - First results of Cepheid variables Ultraviolet spectroscopy of F and G supergiants with IUE. I - First results of Cepheid variables

Jul 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...239..555p&link_type=abstract

Astrophysical Journal, Part 1, vol. 239, July 15, 1980, p. 555-564.

Astronomy and Astrophysics

Astronomy

9

Cepheid Variables, F Stars, G Stars, Satellite-Borne Instruments, Stellar Spectra, Supergiant Stars, Ultraviolet Astronomy, Ultraviolet Spectroscopy, Emission Spectra, Iue, Line Spectra, Stellar Spectrophotometry, Stellar Temperature

Scientific paper

The analysis deals with the bright Cepheids observed from the IUE satellite, over several days, at a speed and spectral resolution suitable to study both the cores of Mg II at 2796 and 2803 A and the presence and strength of the more prominent emission lines in the far ultraviolet. The observations are discussed in some detail. Some qualitative results are examined.

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