Implicit SPH Drag and Dusty Gas Dynamics

1997 ◽  
Vol 138 (2) ◽  
pp. 801-820 ◽  
Author(s):  
J.J. Monaghan
Keyword(s):  
Gas Dynamics ◽  
Dusty Gas ◽  
Implicit Sph

Cometary Dusty Gas Dynamics

2013 ◽  
pp. 433-439
Author(s):  
T. I. Gombosi ◽  
A. KöRöSmezey
Keyword(s):  
Gas Dynamics ◽  
Dusty Gas

scholarly journals Inviscid Flow of Radiation Dusty Gas Dynamics

1981 ◽  
Vol 31 (2) ◽  
pp. 133-142
Author(s):  
S. P. Barnwal ◽  
O. S. Srivastava
Keyword(s):  
Gas Dynamics ◽  
Inviscid Flow ◽  
Dusty Gas

DUSTY GAS-DYNAMICS IN REAL COMETS

Comets ◽  
1982 ◽  
pp. 357-369
Author(s):  
MAX K. WALLIS
Keyword(s):  
Gas Dynamics ◽  
Dusty Gas

Supernovae and interstellar gas dynamics

1967 ◽  
Vol 31 ◽  
pp. 117-119
Author(s):  
F. D. Kahn ◽  
L. Woltjer
Keyword(s):  
Lower Limit ◽  
High Velocity ◽  
Gas Dynamics ◽  
Interstellar Cloud ◽  
Interstellar Gas ◽  
Random Motions ◽  
Relativistic Particles

The efficiency of the transfer of energy from supernovae into interstellar cloud motions is investigated. A lower limit of about 0·002 is obtained, but values near 0·01 are more likely. Taking all uncertainties in the theory and observations into account, the energy per supernova, in the form of relativistic particles or high-velocity matter, needed to maintain the random motions in the interstellar gas is estimated as 1051·4±1ergs.

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