Stark Broadening of several Ne II, Ne III and O III Spectral Lines for the Stark-B Database

Details Stark Broadening of several Ne II, Ne III and O III Spectral Lines for the Stark-B Database Stark Broadening of several Ne II, Ne III and O III Spectral Lines for the Stark-B Database

2012-01-10

arxiv.org/abs/1201.2016v1

Baltic Astronomy, vol. 20, 580-586, 2011

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

Scientific paper

In order to complete Stark broadening data for Ne II, and O III lines, needed for analysis of stellar atmospheres, we determined, within the semiclassical perturbation method, the missing Stark broadening parameters for the broadening by collisions with protons and ionized helium, for 15 Ne II and 5 O III multiplets. Also, electron, proton, and ionized helium impact broadening parameters for an important Ne II multiplet in the visible part of the spectrum, and for three Ne III multiplets, were calculated. The obtained data will be included in the STARK-B database, which is a part of Virtual Atomic and Molecular Data Center.

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