SIMBAD references

In this paper, we present experimental Stark halfwidths of spectral lines of singly ionized oxygen and singly and double ionized silicon. The observed spectral lines were emitted from plasma produced in a small electromagnetically driven T-tube. The plasma electron density was 1.45 x 10²³ m^–3 and the electron temperature was 15 000 K. The obtained results were compared with the available experimental results of other authors, as well as with some theoretical Stark halfwidth values. The obtained results, the analysis of experimental results and the comparison with theoretical results might be of interest in astrophysics. For example, the obtained Stark halfwidths can be useful for abundance determination, the calculation of stellar opacities, the interpretation and modelling of stellar spectra, the estimation of the relative transfer through the stellar plasma, etc.