Does Kozai resonance drive CH Cygni?
S Mikkola, K Tanikawa - The Astronomical Journal, 1998 - iopscience.iop.org
An analysis of the observed radial velocities in the system CH Cygni has been conducted in
the framework of three-body dynamics. The observations and the fact that this star began …
the framework of three-body dynamics. The observations and the fact that this star began …
CH Cygni: TiO molecule as a probe of temperature variations in the atmosphere of the cool component
D Kotnik-Karuza… - … , v. 355, p. 595-602 (2000), 2000 - adsabs.harvard.edu
We report our determination of T vib from band systems of TiO in the visible spectra of the
symbiotic star CH Cygni during its 1987-89 quiescent phase as well as beta And and 30 …
symbiotic star CH Cygni during its 1987-89 quiescent phase as well as beta And and 30 …
The pure rotational spectrum of the ScO (X2Σ+) radical
DT Halfen, J Min, LM Ziurys - Journal of Molecular Spectroscopy, 2017 - Elsevier
The rotational spectrum of ScO (X 2 Σ+) has been measured in the gas phase in the
frequency range 30–493 GHz using a combination of Fourier transform …
frequency range 30–493 GHz using a combination of Fourier transform …
[HTML][HTML] Search for the remnants of the 1977-1986 outburst in the quiescent phase of CH Cygni.
We present the results of spectroscopic measurements of line spectra of the symbiotic star
CH Cygni in the optical region of the EM spectrum. The observations extend over a period of …
CH Cygni in the optical region of the EM spectrum. The observations extend over a period of …
CH Cygni 1987-89: The inactive state as a precursor to the new outburst
In order to help answering the question generally posed for symbiotic stars: are the
apparently inactive periods quiescent at all, or should they be regarded merely as a …
apparently inactive periods quiescent at all, or should they be regarded merely as a …
[HTML][HTML] High velocity gas outflow of the symbiotic star CH Cyg
T Iijima - Astrophysical Letters and Communications, Vol. 34, p …, 1996 - adsabs.harvard.edu
High Velocity Gas Outflow of the Symbiotic Star CH Cyg ADS Classic is now deprecated. It will be
completely retired in October 2019. This page will automatically redirect to the new ADS interface …
completely retired in October 2019. This page will automatically redirect to the new ADS interface …
Atlas of M7III spectral features in the optical
The difficulties encountered in attempts to study the spectra of very late stars inspired us to
prepare this spectral atlas containing essentially spectral features of M7III stars in the optical …
prepare this spectral atlas containing essentially spectral features of M7III stars in the optical …
[PDF][PDF] Conference paper (Received December 23, 1997; accepted March 30, 1998)
D KOTNIK-KARUZA, R JURDANA-ŠEPIČ - researchgate.net
This paper contributes to the ongoing discussion on the nature of the extraordinary star CH
Cygni. A review of our observations of optical spectra of CH Cygni in its inactive period 1987 …
Cygni. A review of our observations of optical spectra of CH Cygni in its inactive period 1987 …
Search for signs of a new outburst in the quiescent state of CH Cygni
A review of our investigations of CH Cygni in its inactive state in the period 1987–1989 is
given. Optical spectra reveal the development of physical conditions in the photosphere of …
given. Optical spectra reveal the development of physical conditions in the photosphere of …
Optical Spectroscopy and Modelling of the Symbiotic Star CH Cygni in the Inactive State
D Kotnik-Karuza… - … Bulletin, vol. 22, no. 1, p …, 1998 - adsabs.harvard.edu
This paper contributes to the ongoing discussion on the nature of the extraordinary star CH
Cygni. A review of our observations of optical spectra of CH Cygni in its inactive period 1987 …
Cygni. A review of our observations of optical spectra of CH Cygni in its inactive period 1987 …