Analysis of the far ultraviolet emission lines in late type stars

Details Analysis of the far ultraviolet emission lines in late type stars Analysis of the far ultraviolet emission lines in late type stars

Oct 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26a...102..207d&link_type=abstract

Astronomy and Astrophysics, vol. 102, no. 2, Oct. 1981, p. 207-211.

Astronomy and Astrophysics

Astrophysics

8

Electron Density (Concentration), Emission Spectra, Far Ultraviolet Radiation, Late Stars, Line Spectra, Spectrum Analysis, Dwarf Stars, Electron Pressure, Iue, Spectral Resolution, Stellar Coronas, Stellar Evolution, Stellar Luminosity, Stellar Temperature

Scientific paper

Far ultraviolet emission lines in a sample of seven stars of spectral type later than F5 and different luminosity class have been analyzed to calculate the electron density and pressure in the formation region of the lines. Three different methods were used. We obtain electron pressures larger than solar for all dwarf stars of the sample. The low resolution observations were made with the IUE satellite.

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