HD113001 - Photometric Separation

Details HD113001 - Photometric Separation HD113001 - Photometric Separation

Aug 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....88..370g&link_type=abstract

Astronomy and Astrophysics, Vol. 88, P. 370, 1980

Astronomy and Astrophysics

Astrophysics

7

Scientific paper

The distance and absolute magnitude of SdO-type stars are very badly known. The existence of a SdO + F binary may therefore bring a solution to the problem.
By using a method already applied in a previous paper (Goy, 1977) we show that the spectral distribution of the F component is exactly similar to that of a normal F 2 V star. The absolute magnitude of the hot star can thus be deduced with good accuracy.

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