High temporal resolution observations of the pulsar microstructure at 102 MHz.

Autor: Kuzmin, A.D., Hamilton, P.A., Shitov, Yu.P., McCulloch, P.M., McConell, D., Pugatchev, V.D.
Předmět:
Zdroj: Monthly Notices of the Royal Astronomical Society; 10/1/2003, Vol. 344 Issue 4, p1187, 6p
Abstrakt: Reports observations of the microstructure of seven pulsars at 102 MHz with a time resolution of up to one microsecond. Detection of fine pulse structure with a µs time-scale for all seven pulsars; Indication that interstellar scattering does not broaden the µ time-scale pulsar microstructure; Shorter structure of a time-scale than the interstellar scatter broadening; Dispersion measure; Train of quasi-periodic micropulses with an exponentially damped envelope.
Databáze: Complementary Index