Internal consistency test about δm1 metallicity index for SX Phe and high amplitude δ Sct stars.

Details Internal consistency test about δm1 metallicity index for SX Phe and high amplitude δ Sct stars. Internal consistency test about δm1 metallicity index for SX Phe and high amplitude δ Sct stars.

Nov 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990rmxaa..21..386r&link_type=abstract

Revista Mexicana de Astronomia y Astrofisica, Vol. 21, p. 386 - 388

Astronomy and Astrophysics

Astronomy

4

Delta Scuti Stars: Light Curves, Delta Scuti Stars: Periods, Delta Scuti Stars: Metal Abundances

Scientific paper

The authors have carried out a systematic study of the behaviour of the δm1 metallicity index for SX Phe and high amplitude δ Sct stars. It is shown to be different for the two samples of stars. The δm1 parameter increases or decreases towards the minimum light for the first or second sample, respectively. The m1 index variation is larger when the metal abundance of the star is smaller.

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