Atomization of Liquids in High Velocity Gas Streams

1948 ◽  
Vol 40 (1) ◽  
pp. 67-74 ◽  
Author(s):  
H. C. Lewis ◽  
D. G. Edwards ◽  
M. J. Goglia ◽  
R. I. Rice ◽  
L. W. Smith
Keyword(s):  
1984 ◽  
Vol 80 ◽  
pp. 95-99
Author(s):  
W. C. Seitter

AbstractSpectroscopic observations through most of the eclipse cycle of BT Mon reveal the presence of both low and high velocity gas streams. Acceleration through a Laval-nozzle-effect at the inner Lagrangian point of the system and powering of the emission lines through kinetic energy losses of Coriolis deflected and subsequently colliding gas streams are considered as possible mechanisms at work in the system.


2009 ◽  
Vol 60 (2) ◽  
pp. 139-162 ◽  
Author(s):  
Ernest F. Fiock ◽  
Andrew I. Dahl
Keyword(s):  

1978 ◽  
Vol 10 (6) ◽  
pp. 631-635
Author(s):  
Yu. G. Veksler ◽  
V. G. Sorokin ◽  
V. P. Lesnikov ◽  
Yu. A. Belykh

1954 ◽  
Vol 5 (4) ◽  
pp. 195-217 ◽  
Author(s):  
D. B. Spalding ◽  
B. S. Tall

SummaryThe first object of this paper is to show the concordance between three different theoretical approaches to flame stabilisation and to compare published experimental data with the theoretical predictions. Good agreement between the theory and experimental results is obtained. The second object is to show that, at low pressures, the predictions of these theories must be qualified in view of the increasing importance of heat losses from the flame region. It is shown that there must exist a minimum pressure below which a flame cannot be maintained in a given combustible mixture, irrespective of the rate of flow of the mixture, unless heat losses are entirely eliminated.


1966 ◽  
Vol 25 ◽  
pp. 93-97
Author(s):  
Richard Woolley

It is now possible to determine proper motions of high-velocity objects in such a way as to obtain with some accuracy the velocity vector relevant to the Sun. If a potential field of the Galaxy is assumed, one can compute an actual orbit. A determination of the velocity of the globular clusterωCentauri has recently been completed at Greenwich, and it is found that the orbit is strongly retrograde in the Galaxy. Similar calculations may be made, though with less certainty, in the case of RR Lyrae variable stars.


1967 ◽  
Vol 31 ◽  
pp. 117-119
Author(s):  
F. D. Kahn ◽  
L. Woltjer

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.


1914 ◽  
Vol 111 (5) ◽  
pp. 82-82
Author(s):  
Frank C. Perkins
Keyword(s):  

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