Rydberg Atomic Complexes in Astrophysical Plasmas

In this contribution, we further investigate processes which include Rydberg atomic complexes important for the different astrophysical environments. The range of the used physical parameters covers the area important for plasma modeling from astrophysical standpoint (white dwarfs, central stars of planetary nebulae, etc). Naturally, these results can be of interest and use in investigation of different laboratory plasmas. Also, we present overview of future developments and needs in the areas of Rydberg collisional processes.