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Blanketing Hypothesis and Light Variations of HD 27309
1986
International Astronomical Union Colloquium
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AbstractThe influence of variable blanketing on the photometric variations of hot, silicon Ap star HD 27309 has been estimated. Spectrum variations in the visible are not the principal reason for the observed light variability, but flux redistribution from UV into visible fit well the observational data. An reference is made on the fulfillment of the variable blanketing assumptions at least for silicon Ap stars.
doi:10.1017/s0252921100091673
fatcat:ag6t62sn65fltd5nwtxa6vgtoi