A Comment on 'Far Ultraviolet Photometry of Orion Stars' by G. R. Carruthers

Details A Comment on 'Far Ultraviolet Photometry of Orion Stars' by G. R. Carruthers A Comment on 'Far Ultraviolet Photometry of Orion Stars' by G. R. Carruthers

Jul 1970

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1970ap%26ss...8...50m&link_type=abstract

Astrophysics and Space Science, Volume 8, Issue 1, pp.50-52

Astronomy and Astrophysics

Astrophysics

9

Scientific paper

It is shown that the ultraviolet flux-deficiency, recently discovered by Carruthers, in early-type supergiants compared to dwarfs of the same spectral type can be explained in terms of the effects of differences in surface-gravity and effective temperature between stars of these two luminosity classes. It thus appears that this deficiency does not represent a serious discrepancy between theory and observation.

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