Crab giant pulses at low frequencies

Details Crab giant pulses at low frequencies Crab giant pulses at low frequencies

Feb 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012a%26a...538a...7k&link_type=abstract

Astronomy & Astrophysics, Volume 538, id.A7

Astronomy and Astrophysics

Astrophysics

Radiation Mechanisms: Non-Thermal, Scattering

Scientific paper

We report observations of the Crab pulsar at frequencies in the range of 110-180 MHz. The combination of coherent dedispersion and the narrow synthesised beam of the Westerbork Synthesis Radio Telescope resulted in a sensitive observation. Our improved sensitivity and resolution allow us to confirm the presence of a precursor to the interpulse at these frequencies. We also detected more than 1000 giant pulses and find that the interpulse precursor component shows no giant pulse emission. Therefore, we attribute it to a similar emission source as the precursor to the mainpulse. Together these precursors might be the normal emission seen from the majority of radio pulsars. From the dispersion-free giant pulses, we find that the emission rate is ~10-20 × 10-3 s-1 and the scatter timescale in the range of ~1.5-5.6 ms. We further find that the radio flux of the pulsar is 6-11 Jy in this frequency range.

Affiliated with

Also associated with

No associations

Rating

Crab giant pulses at low frequencies 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 Crab giant pulses at low frequencies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Crab giant pulses at low frequencies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-887319