scholarly journals The radiation gas dynamics of planetary nebulae. 4. From the Owl to the Eskimo

1994 ◽  
Vol 430 ◽  
pp. 800 ◽  
Author(s):  
Adam Frank ◽  
Garrelt Mellema
Keyword(s):  
Gas Dynamics ◽  
Planetary Nebulae ◽  
Radiation Gas Dynamics

scholarly journals Evolution and Gas Dynamics of Planetary Nebulae

1978 ◽  
Vol 76 ◽  
pp. 251-261 ◽  
Author(s):  
William G. Mathews
Keyword(s):  
Gas Dynamics ◽  
Planetary Nebulae ◽  
Central Star ◽  
Made In

Since the last IAU Symposium on Planetary Nebulae at Tatranska-Lomnica, a number of significant theoretical and observational advances have been made in the study of nebular dynamics. The following review emphasizes the evolution of nebulae after they have been ejected from the central star and have become optically thin to most radiation.

Methods of solving one-dimensional problems of radiation gas dynamics. II

1973 ◽  
Vol 13 (5) ◽  
pp. 244-254
Author(s):  
V.F. Bashurin ◽  
Yu.V. Varlamov ◽  
V.Ya. Gol'din ◽  
V.N. Chetverushkin
Keyword(s):  
Gas Dynamics ◽  
One Dimensional ◽  
Radiation Gas Dynamics

scholarly journals On modeling the problems of high-temperature radiation gas dynamics

1984 ◽  
pp. 1-17
Author(s):  
Vladimir Yakovlevich Gol’din ◽  
Dinamika Alekseevna Gol'dina ◽  
Andrey Vasilievich Kolpakov ◽  
Alexander Victorovich Shilkov
Keyword(s):  
High Temperature ◽  
Energy Density ◽  
Numerical Methods ◽  
Mathematical Models ◽  
Gas Dynamics ◽  
Radiation Energy ◽  
High Radiation ◽  
Radiation Energy Density ◽  
Temperature Radiation ◽  
Radiation Gas Dynamics

Mathematical models of High-Temperature Radiation Gas Dynamics (HTRGD) are considered. The possibility of instability of contact boundaries at a high radiation energy density is shown. Equations of the three-temperature approximation are consistently derived. Numerical methods for solving the problems of HTRGD are discussed.

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