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Fig. 7


Upper plot: emerging flux from a reference model atmosphere (εMg = −4.1, εSi = −3.7, εCr = −4.4, εMn = −5.7, and εFe = −4.2). Lower plot: difference between the emerging flux from the model atmospheres with higher abundance of the selected element by a factor of 10 and the flux from a reference model. All fluxes were smoothed by a Gaussian filter with a dispersion of 10 Å to show the changes in continuum. The passbands of the uvby photometric system are also denoted.

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