New Views of the Vela Pulsar Jet

1998 ◽  
pp. 221-227
Author(s):  
C. B. Markwardt ◽  
H. B. Ögelman
Keyword(s):  
Astrophysics ◽  
2007 ◽  
Vol 50 (2) ◽  
pp. 144-156 ◽  
Author(s):  
D. M. Sedrakian ◽  
M. V. Hayrapetyan ◽  
L. R. Sedrakian
Keyword(s):  

Author(s):  
Armando Manzali ◽  
Andrea De Luca ◽  
Patrizia A. Caraveo
Keyword(s):  

1971 ◽  
pp. 217-221
Author(s):  
M. M. Komesaroff ◽  
P. A. Hamilton ◽  
J. G. Ables

1998 ◽  
pp. 211-219 ◽  
Author(s):  
L. Kuiper ◽  
W. Hermsen ◽  
V. Schönfelder ◽  
K. Bennett ◽  
A. Connors
Keyword(s):  

1996 ◽  
Vol 160 ◽  
pp. 21-22
Author(s):  
R. Wietfeldt ◽  
W. Van Straten ◽  
D. Del Rizzo ◽  
N. Bartel ◽  
W. Cannon ◽  
...  

AbstractThe phase-coherent recording of pulsar data and subsequent software dispersion removal provide a flexible way to reach the limits of high time resolution, useful for more precise pulse timing and the study of fast signal fluctuations within a pulse. Because of the huge data rate and lack of adequate recording and computing capabilities, this technique has been used mostly only for small pulsar data sets. In recent years, however, the development of very capable, reasonably inexpensive high-speed recording systems and computers has made feasible the notion of pulsar baseband recording and subsequent processing with a workstation/computer. In this paper we discuss the development of a phase-coherent baseband processing system for radio pulsar observations. This system is based on the S2 VLBI recorder developed at ISTS/York University in Toronto, Canada. We present preliminary first results for data from the Vela pulsar, obtained at Parkes, Australia, and processed at ISTS/York University, and discuss plans for future developments.


2000 ◽  
Vol 177 ◽  
pp. 215-218 ◽  
Author(s):  
J.-P. Macquart ◽  
S. Johnston ◽  
M. Walker ◽  
D. Stinebring

AbstractWe have measured the properties of the diffractive scintillation toward the Vela pulsar under the extremely strong scattering conditions encountered at 660 MHz. We obtain a decorrelation bandwidth ofvd= 244±4 Hz and diffractive decorrelation timescale oftdiff= 3.3±0.3s. Our measurement of the modulation indicesm= 0.87±0.003±0.05 andm= 0.93±0.03±0.05 (one For each polarization stream), are at variance with the modulation index of the Vela pulsar obtained at 2.3 GHz by Gwinn et al. (F997)ifthe deviation from a modulation index of unity is ascribed to a source size effect.


2011 ◽  
Vol 737 (2) ◽  
pp. 93 ◽  
Author(s):  
J. Abadie ◽  
B. P. Abbott ◽  
R. Abbott ◽  
M. Abernathy ◽  
T. Accadia ◽  
...  

1974 ◽  
Vol 190 ◽  
pp. 667 ◽  
Author(s):  
D. C. Backer

1976 ◽  
Vol 203 ◽  
pp. 213 ◽  
Author(s):  
M. Ruderman
Keyword(s):  

1984 ◽  
Vol 278 ◽  
pp. 791 ◽  
Author(s):  
M. A. Alpar ◽  
P. W. Anderson ◽  
D. Pines ◽  
J. Shaham

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