Speaker
Nawamin Intrarat
(Chiang Mai University)
Description
Pulsars are rapidly rotating and highly magnetized neutron stars that radiate non-thermal radio beams from their poles. The radio emission of pulsars usually remains stable in the averaged intensity of ~1,000 pulses or more, but some pulsars exhibit interesting features in emission variations on short and long timescales. In this research, we report the phase-resolved pulse-to-pulse energy distribution of pulsar PSRJ1825-0935 and found that the pulse profile’s main component energy distribution is well described by a log-normal distribution. This pulsar has two different emission modes, B and Q modes, and we analyze the energy distribution of each mode energy separately.
Keywords: Pulsar, energy distribution
Author
Nawamin Intrarat
(Chiang Mai University)
Co-author
Phrudth Jaroenjittichai
