A Study of the Near‐Ultraviolet Spectrum of Vega
A Study of the Near‐Ultraviolet Spectrum of Vega
UV, optical, and near-IR spectra of Vega have been combined to test our understanding of stellar atmospheric opacities, and to examine the possibility of constraining chemical abundances from low-resolution UV fluxes. We have carried out a detailed analysis assuming Local Thermodynamic Equilibrium (LTE) to identify the most important contributors to …