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Cited article:

High-velocity equatorial mass ejections and some other spectroscopic phenomena of the symbiotic star CH Cygni in an active stage

T. Iijima, H. Naito and S. Narusawa
Astronomy & Astrophysics 622 A45 (2019)
https://doi.org/10.1051/0004-6361/201833858

Comparison of observed and predicted Lyα and ultraviolet lines in galaxy spectra at redshiftsz < 3.7, adopting photoionization + shock composite models

M. Contini
Monthly Notices of the Royal Astronomical Society 452 (4) 3795 (2015)
https://doi.org/10.1093/mnras/stv1451

OUTFLOWS FROM ACTIVE GALACTIC NUCLEI: KINEMATICS OF THE NARROW-LINE AND CORONAL-LINE REGIONS IN SEYFERT GALAXIES,

F. Müller-Sánchez, M. A. Prieto, E. K. S. Hicks, et al.
The Astrophysical Journal 739 (2) 69 (2011)
https://doi.org/10.1088/0004-637X/739/2/69

The spectral energy distribution of D-type symbiotic stars: the role of dust shells

R. Angeloni, M. Contini, S. Ciroi and P. Rafanelli
Monthly Notices of the Royal Astronomical Society 402 (3) 2075 (2010)
https://doi.org/10.1111/j.1365-2966.2009.16067.x

The symbiotic system CH Cygni: An analysis of the shocked nebulae at different epochs

M. Contini, R. Angeloni and P. Rafanelli
Astronomische Nachrichten 330 (8) 816 (2009)
https://doi.org/10.1002/asna.200911225