Drifting sub-pulses in two newly discovered pulsars

1Citations
Citations of this article
5Readers
Mendeley users who have this article in their library.
Get full text

Abstract

We have detected the rare phenomenon of stable, drifting sub-pulse behaviour in two pulsars discovered in the recent Swinburne intermediate latitude pulsar survey. The pulsars, PSR J1231 - 47 and PSR J1919+0134, have approximate periods (P) of 1.873 and 1.6039s respectively. Both pulsars have multicomponent profiles, and distinct drifting is observed across them. We have identified a single drift mode in both pulsars: the drift rate for PSR J1231 - 47 being 5.4(1) ms P-1 and 5.8(2) ms P-1 for PSR 1919+0134. The drifting is linear across the profile with no departure from linearity at the edges within the sensitivity of our observations.

Cite

CITATION STYLE

APA

Ord, S. M., Edwards, R., & Bailes, M. (2001). Drifting sub-pulses in two newly discovered pulsars. Monthly Notices of the Royal Astronomical Society, 328(3), 911–913. https://doi.org/10.1046/j.1365-8711.2001.04946.x

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free