Spectroscopic survey of the far-ultraviolet /1160-1700 A/ emissions of Capella

Details Spectroscopic survey of the far-ultraviolet /1160-1700 A/ emissions of Capella Spectroscopic survey of the far-ultraviolet /1160-1700 A/ emissions of Capella

Apr 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...205l..35v&link_type=abstract

Astrophysical Journal, vol. 205, Apr. 1, 1976, pt. 2, p. L35-L38.

Astronomy and Astrophysics

Astrophysics

23

Far Ultraviolet Radiation, Late Stars, Spectral Energy Distribution, Stellar Spectra, Ultraviolet Spectroscopy, Astronomical Spectroscopy, Energy Spectra, Line Spectra, Lyman Alpha Radiation, Solar Spectra, Spectrographs, X Ray Sources

Scientific paper

A far-ultraviolet spectral survey of Capella (Alpha Aur, G5 III + G0 III) has been obtained using a highly sensitive rocketborne spectrograph with a microchannel plate detector. The spectral distribution is very similar to that of the sun; however, if the line surface fluxes are due to the primary (G5 III), then, except for Ly-alpha, they are about an order of magnitude greater than those of the quiet sun

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