Thirteen Drift Bands in PSR B0826–34

Esamdin, Ali; Lyne, A. G.; Krämer, M.; Graham‐Smith, Francis; Manchester, R. N.

doi:10.1017/s0074180900181331

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“…This may also be possible in PSR J1012+5307 (Kramer et al 1999). This effect has already been observed for normal pulsar B0826-34 (Biggs et al 1985;Esamdin et al 2003).…”

Section: Discussion and Summarysupporting

confidence: 62%

Observations of millisecond pulsars at 8.35 GHz

Maron

Kijak

Wielebinski

2003

A&A

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Abstract. New pulsar observations at 8.35 GHz with the newly built highly sensitive receiver of the Effelsberg 100-m Radio Telescope are reported. They resulted in the first detection of 3 millisecond pulsars J1713+0747, B1855+09 and J2145-0750 at this high frequency. The measured flux densities indicate that the spectrum of all three pulsars follows a single power law. PSR B1855+09 shows a significant increase of the Interpulse-to-Mainpulse amplitude ratio at high frequencies.

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“…This may also be possible in PSR J1012+5307 (Kramer et al 1999). This effect has already been observed for normal pulsar B0826-34 (Biggs et al 1985;Esamdin et al 2003).…”

Section: Discussion and Summarysupporting

confidence: 62%