HD94033 and the mass of SX phoenicis type variables

Details HD94033 and the mass of SX phoenicis type variables HD94033 and the mass of SX phoenicis type variables

Jun 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989cha%26a..13..213j&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 13, Issue 2, p. 213-215.

Astronomy and Astrophysics

Astrophysics

Scientific paper

Using some new observed data it is shown that the binary assumption for
HD 94033 is believable. A brief discussion on the question of the mass
of SX Phe follows. I believe that the mass of this type of variable star
is in the range from about 0.6 to 0.9 suns, and the mass of AI Vel type
stars with normal metal content is between 1.5 and 2.0 suns.

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