Charge Transfer Scattering in High‐Velocity Neutral Particle Production

1962 ◽  
Vol 33 (2) ◽  
pp. 739-743 ◽  
Author(s):  
Byron L. Johnson
1983 ◽  
Vol 103 ◽  
pp. 219-227
Author(s):  
J. Patrick Harrington

Computed models are now recognized as useful tools for interpretation of the spectra of planetary nebulae. However, even the most detailed models need geometrical parameters such as filling factors which are poorly determined by observations. Some effects may be seen more clearly by modeling the stratification than by just using total fluxes. A simple model for NGC 6720 is presented which reproduces the behavior of (Ne III) λ3869 observed by Hawley and Miller (1977), clearly showing the effects of charge transfer. The behavior of C II λ4267 remains puzzling. Finally, we comment on the interaction of high velocity stellar winds with nebular shells. Non-equilibrium particle distributions at the contact between the shocked stellar wind and the nebula may result in the rapid cooling of the shocked gas.


1975 ◽  
Vol 35 (3) ◽  
pp. 142-145 ◽  
Author(s):  
Margaret Alston-Garnjost ◽  
J. Erwin ◽  
J. H. Klems ◽  
W. Ko ◽  
R. L. Lander ◽  
...  

1974 ◽  
Author(s):  
K. Jaeger ◽  
/Argonne ◽  
R. Ammar ◽  
R. Davis ◽  
L. Loos ◽  
...  

1979 ◽  
Vol 20 (3) ◽  
pp. 605-614 ◽  
Author(s):  
R. D. Kass ◽  
W. Ko ◽  
R. L. Lander ◽  
W. Michael ◽  
D. E. Pellett ◽  
...  

Author(s):  
K. Wohrer ◽  
F.Ben Salah ◽  
J.P. Rozet ◽  
A. Chetioui ◽  
A. Touati ◽  
...  

2019 ◽  
Vol 208 ◽  
pp. 05008
Author(s):  
Qi-Dong Zhou

LHCf is an experiment dedicated to verify the hadronic interaction models by measuring the forward neutral particle production at the LHC. Corresponding data are very important for understanding hadronic interactions occurring in air-shower development. According to the current LHCf results, no simulation model predicts the LHCf data perfectly. In order to provide more specific data, it is necessary to classify the LHCf observables into specific interaction types: diffraction or non-diffraction. Combining the information of ATLAS, LHCf is able to classify these specific interaction types experimentally. Especially, the ATLAS-LHCf joint experiment will have the unique sensitivity to low mass diffraction. LHCf and ATLAS have succeeded in the common data-taking in p-p collisions at √s = 13 TeV. We will report the first ATLAS-LHCf joint analysis result and discuss the impact of the corresponding joint analysis result to the determination of mass composition of ultra-high energy cosmic-rays.


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