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The photospheric lines in the visual region of the cool magnetic CP star HR 7575 have been analyzed using a high-dispersion spectrogram obtained at the Dominion Astrophysical Observatory. The fully line-blanketed ATLAS9 model atmospheres of 10-times the solar metal content were employed to calculate the elemental abundances. The effective temperature Teff, derived from the optical and ultraviolet ...

Analysis of the Photospheric Lines of the Magnetic CP Star HR 7575