PSR 1133+16 - Determination of the dispersion measure and the locations of the emitting regions

Details PSR 1133+16 - Determination of the dispersion measure and the locations of the emitting regions PSR 1133+16 - Determination of the dispersion measure and the locations of the emitting regions

May 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...109..340k&link_type=abstract

Astronomy and Astrophysics, vol. 109, no. 2, May 1982, p. 340-343.

Astronomy and Astrophysics

Astrophysics

24

Electron Density (Concentration), Pulsars, Stellar Radiation, Time Lag, Wave Dispersion, Cross Correlation, Emission Spectra, Lorentz Force, Spectral Correlation

Scientific paper

Clear correlation is found for the microstructure of PSR 1133+16 observed simultaneously at 67.5, 78.9, and 102.55 MHz. The time delay follows the dispersion relation, suggesting a dispersion measure of DM equals 4.8413 + or - 0.0003/cu cm pc. This precise determination of dispersion measure makes it possible to measure the retardation and aberration time of pulses emitted simultaneously at 102.55 and 1700 MHz; from these the radii of the emission regions at these frequencies may be computed. It is also possible to estimate the limits of the Lorentz factor and the electron density of the emitting plasma.

Affiliated with

Also associated with

No associations

Rating

PSR 1133+16 - Determination of the dispersion measure and the locations of the emitting regions does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with PSR 1133+16 - Determination of the dispersion measure and the locations of the emitting regions, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and PSR 1133+16 - Determination of the dispersion measure and the locations of the emitting regions will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1099933