Asymmetry of Lines in the Spectra of the Sun and Solar-Type Stars

[1] Allende Prieto C.(2002)Signatures of convection in the spectrum of Procyon: Fundamental parameters and iron abundance Astrophys. J. 567 544-565

[2] Asplund M.(1998)Fe I line shifts in the optical spectrum of the Sun Astron. Astrophys., Suppl. Ser. 129 41-44

[3] García López R. J.(1999)Spectroscopic observations of convective patterns in the atmospheres of metal-poor stars Astrophys. J. 526 991-1000

[4] Lambert D. L.(2013)Convective line shifts for the GAIA RVS from the CIFIST 3D model atmosphere grid Astron. Astrophys. 550 A103-742

[5] Allende Prieto C.(2000)Line formation in solar granulation. I. Fe line shapes, shifts and asymmetries Astron. Astrophys. 359 729-656

[6] García López R. J.(1994)Three-dimensional hydrodynamic models of solar granulation and their application to a spectral analysis problem Astron. Astrophys. 291 635-241

[7] Allende Prieto C.(1984)Asymmetries and wavelengths of solar spectral lines and the solar rotation determined from Fourier-transform spectra Sol. Phys. 93 219-72

[8] García López R. J.(2015)Convection structure in the solar photosphere at granulation and mesogranulation scales Kinematics Phys. Celestial Bodies 31 65-74

[9] Lambert D. L.(2013)Three-dimensional simulations of near-surface convection in main-sequence stars. II. Properties of granulation and spectral lines Astron. Astrophys. 558 A49-224

[10] Gustafsson B.(1997)Absolute shifts of Fe I and Fe II lines in solar active regions (disk center) Kinematics Phys. Celestial Bodies 13 65-213

[1] Allende Prieto C.(2002)Signatures of convection in the spectrum of Procyon: Fundamental parameters and iron abundance Astrophys. J. 567 544-565

[2] Asplund M.(1998)Fe I line shifts in the optical spectrum of the Sun Astron. Astrophys., Suppl. Ser. 129 41-44

[3] García López R. J.(1999)Spectroscopic observations of convective patterns in the atmospheres of metal-poor stars Astrophys. J. 526 991-1000

[4] Lambert D. L.(2013)Convective line shifts for the GAIA RVS from the CIFIST 3D model atmosphere grid Astron. Astrophys. 550 A103-742

[5] Allende Prieto C.(2000)Line formation in solar granulation. I. Fe line shapes, shifts and asymmetries Astron. Astrophys. 359 729-656

[6] García López R. J.(1994)Three-dimensional hydrodynamic models of solar granulation and their application to a spectral analysis problem Astron. Astrophys. 291 635-241

[7] Allende Prieto C.(1984)Asymmetries and wavelengths of solar spectral lines and the solar rotation determined from Fourier-transform spectra Sol. Phys. 93 219-72

[8] García López R. J.(2015)Convection structure in the solar photosphere at granulation and mesogranulation scales Kinematics Phys. Celestial Bodies 31 65-74

[9] Lambert D. L.(2013)Three-dimensional simulations of near-surface convection in main-sequence stars. II. Properties of granulation and spectral lines Astron. Astrophys. 558 A49-224

[10] Gustafsson B.(1997)Absolute shifts of Fe I and Fe II lines in solar active regions (disk center) Kinematics Phys. Celestial Bodies 13 65-213