Use of Electron Probes in the Study of Recombination Radiation

1964 ◽  
Vol 35 (8) ◽  
pp. 2439-2442 ◽  
Author(s):  
David B. Wittry ◽  
David F. Kyser
Keyword(s):  
Recombination Radiation

Recombination radiation in natural and compensated GaSb

1970 ◽  
Vol 2 (4) ◽  
pp. 779-784 ◽  
Author(s):  
M. D'Olne Campos ◽  
A. Gouskov ◽  
L. Gouskov ◽  
J.-C. Pons
Keyword(s):  
Recombination Radiation

Infrared Television Microscope for the Investigation of Recombination Radiation and the Optical Properties of Semiconductors

1970 ◽  
pp. 98-101
Author(s):  
N. L. Artem’ev ◽  
V. S. Bagaev ◽  
O. V. Gogolin ◽  
Yu. A. Efimov ◽  
B. D. Kopylovskii
Keyword(s):  
Optical Properties ◽  
Recombination Radiation

Manifestation of exitonic effects in the magneto-oscillations of the intensity of the recombination radiation of 2D electrons

JETP Letters ◽  
1996 ◽  
Vol 64 (10) ◽  
pp. 774-779 ◽  
Author(s):  
O. V. Volkov ◽  
V. E. Zhitomirskii ◽  
I. V. Kukushkin ◽  
K. von Klitzing ◽  
K. Eberl
Keyword(s):  
Recombination Radiation

scholarly journals The formation and early evolution of the Milky Way

1985 ◽  
Vol 106 ◽  
pp. 603-610
Author(s):  
S. Michael Fall
Keyword(s):  
Galaxy Formation ◽  
Milky Way ◽  
Chemical Compositions ◽  
Fundamental Plane ◽  
Recombination Radiation ◽  
The Galaxy ◽  
Comprehensive Picture ◽  
Broad Outline ◽  
Kinematic Properties ◽  
Collapse Phase

In broad outline, the traditional picture for the formation of the Milky Way can be summarized as follows. The proto-galaxy consisted of a slowly rotating cloud of metal-free gas that cooled by bremsstrahlung and recombination radiation. As the internal pressure of the gas decreased, it collapsed in stages with smaller dimensions, faster rotation velocities and flatter shapes until it reached centrifugal support in a fundamental plane. At the same time, the gas was progressively depleted by the formation of stars and enriched with heavy elements by the ejecta from previous generations. The result is a general correlation between the kinematic properties, chemical compositions and relative ages of the stellar populations within the Galaxy. This picture was formulated at the Vatican symposium by Oort (1958) and others and was elaborated by Eggen, Lynden-Bell & Sandage (1962), Sandage, Freeman & Stokes (1970), Gott & Thuan (1976), Larson (1976) and others. Much of the recent work on galaxy formation has been an attempt to extend these ideas to a more comprehensive picture that includes large quantities of dark matter. The purpose of this article is to review several topics concerning the collapse phase in the evolution of the Milky Way.

A VUV Recombination Radiation Experiment in a Fast Dynamic Z-Pinch

1994 ◽  
Author(s):  
P. Hagen ◽  
T. Wagner ◽  
M. Stetter ◽  
J. Christiansen ◽  
R. Tkotz ◽  
...  
Keyword(s):  
Recombination Radiation ◽  
Z Pinch ◽  
Fast Dynamic
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