PSR B0826-34: Sometimes a rotating radio transient
Abstract
We report on the detection of sporadic, strong single pulses co-existing with a periodic weak emission in the duration of weak mode of PSR B0826-34. The intensities and durations of these pulses are comparable with that of the sub-pulses in the strong mode, and these pulses are distributed within the phase ranges of the main-pulse and interpulse of the strong-mode average profile. These results suggest that there are most possibly sporadic, very short timescale turn-on of strong-mode emission during the weak-mode state of the pulsar. The emission features of the bursts of strong pulses of PSR B0826-34 during its weak-mode state are similar to those of the rotating radio transients (RRATs). PSR B0826-34 is the second pulsar known which oscillates between pulsar-like and RRAT-like modes.
Keywords
Cite
@article{arxiv.1209.5831,
title = {PSR B0826-34: Sometimes a rotating radio transient},
author = {A. Esamdin and D. Abdurixit and R. N. Manchester and H. B. Niu},
journal= {arXiv preprint arXiv:1209.5831},
year = {2012}
}
Comments
11 pages, 4 figures; 2012, ApJ, 759, L3