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RH-SB

broad.c file with new evaluation of quadratic Stark effect for certain spectral lines (till now, only Mg II h,k and triplets) in RH code . To use it, just replace the broad.c file in your main directory of RH code.

This is a small change to let your RH code use Mg II Stark widths calculated by semi-classical perturbation theory. Besides, you can add some other lines like Si IV with a little effort.

Tested on RH1.5D, should also work on 1D verson (rhf1d).

Have fun!

Some references & Links:

RH1.5D Uitenbroek 2001, Pereira & Uitenbroek 2015

Zhu, Y., Kowalski, A. F., Tian, H., et al. 2019, ApJ, 879, 19 ADS

STARK-B Sahal-Bréchot, S., Dimitrijević, M.S., Moreau N., 2018. STARK-B database, online. http://stark-b.obspm.fr August 29, 2018. Observatory of Paris, LERMA and Astronomical Observatory of Belgrade