Quasi-Stellar Source, 3C 273 B: Variability in Radio Emission

Science ◽  
1965 ◽  
Vol 150 (3692) ◽  
pp. 78-79 ◽  
Author(s):  
G. B. Field
Keyword(s):  
Radio Emission ◽  
Stellar Source

Quasi-Stellar Source, 3C 273 B: Variability in Radio Emission

Science ◽  
1965 ◽  
Vol 150 (3692) ◽  
pp. 78-79
Author(s):  
George B. Field
Keyword(s):  
Radio Emission ◽  
Stellar Source

Nonlinear Phase Radio-Range Station for Measuring Distance to Radio Emission Sources

2007 ◽  
Vol 66 (1) ◽  
pp. 63-67
Author(s):  
N. I. Kozachek ◽  
Vladimir B. Avdeev ◽  
D. V. Senkevich ◽  
S. N. Panychev
Keyword(s):  
Radio Emission ◽  
Emission Sources ◽  
Nonlinear Phase ◽  
Radio Range

A Search for Radio Emission at the Bottom of the Main Sequence and Beyond

1999 ◽  
Vol 118 (3) ◽  
pp. 1369-1372 ◽  
Author(s):  
Anita Krishnamurthi ◽  
Giuseppe Leto ◽  
Jeffrey L. Linsky
Keyword(s):  
Radio Emission ◽  
Main Sequence

scholarly journals Magnetospheric Structure of Rotation-Powered Neutron Stars

1992 ◽  
Vol 128 ◽  
pp. 56-77 ◽  
Author(s):  
Jonathan Arons
Keyword(s):  
Radio Emission ◽  
Gamma Radiation ◽  
Heavy Ions ◽  
Theoretical Work ◽  
Future Research ◽  
Observational Constraints ◽  
Polar Caps ◽  
Recent Theoretical Work ◽  
Density Flow ◽  
Promising Avenue

AbstractI survey recent theoretical work on the structure of the magnetospheres of rotation-powered pulsars, within the observational constraints set by their observed spindown, their ability to power synchrotron nebulae and their ability to produce beamed collective radio emission, while putting only a small fraction of their energy into incoherent X- and gamma radiation. I find no single theory has yet given a consistent description of the magnetosphere, but I conclude that models based on a dense outflow of pairs from the polar caps, permeated by a lower density flow of heavy ions, are the most promising avenue for future research.

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