Geneva Seven-Colour Photometry and Frequency Analysis of the Delta-Scuti Star HD105513

Details Geneva Seven-Colour Photometry and Frequency Analysis of the Delta-Scuti Star HD105513 Geneva Seven-Colour Photometry and Frequency Analysis of the Delta-Scuti Star HD105513

Mar 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26a...283..835h&link_type=abstract

Astronomy and Astrophysics, Vol. 283, NO. 3/MAR(III), P. 835, 1994

Astronomy and Astrophysics

Astrophysics

1

Stars: & Sct- Stars: Oscillations Of- Stars: Individual: Hd 105513

Scientific paper

Photometric observations in the Geneva system of the late-A star HD 105513 show that this star is a δ Scuti variable. Four pulsation frequencies have been extracted from the light curves: f0 = 6.85592±0.00003, f1 = 6.63878±0.00003, f2 = 6.89023±0.00005, and f3 = 6.45861±0.00007, in cycles per day. All four pulsation modes probably are non-radial.

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