Metallicity of the star HD80290(F3V)
Keywords:
F spectral class giant stars, fundamental parameters of starsAbstract
The atmospheres of the HD80290(F3V) star of the F spectral class were studied using the model and parallax methods. The effective temperatures Teff and surface of gravity g of stars were determined based on a comparison of the observed and theoretically calculated values of the photometric quantity [c1] and the equivalent widths of the spectral lines of the hydrogen Balmer series and the use of parallax. Based on the FeII lines, the microturbulence
