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We present new results from high sensitivity GMRT observations of PSR B0826-34. We provide a model to explain the observed subpulse drift properties of this pulsar, including the apparent reversals of the drift direction. In this model, PSR…

Astrophysics · Physics 2009-11-10 Y. Gupta , J. Gil , J. Kijak , M. Sendyk

Pulsars are known to manifest complex phenomena, such as nulling, sub-pulse drifting, and periodicity. Within the purview of this investigation, we have harnessed the wavelet analysis technique to scrutinize the multifaceted periodicities…

High Energy Astrophysical Phenomena · Physics 2024-03-19 Peng-Fu Tian , Ping Zhang , Wen Yang , Wei Wang , Pei Wang

We present a detailed single-pulse study of the long-period pulsar PSR J2129+4119 using high-sensitivity FAST observations. Despite locating well below the traditional death line, the pulsar exhibits sustained and multi-modal emission…

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)…

Astrophysics · Physics 2009-11-07 S. M. Ord , R. Edwards , M. Bailes

A large sample of pulsars was observed as part of the Meterwavelength Single-pulse Polarimetric Emission Survey. We carried out a detailed fluctuation spectral analysis which revealed periodic features in 46% pulsars including 22 pulsars…

High Energy Astrophysical Phenomena · Physics 2016-12-14 Rahul Basu , Dipanjan Mitra , George I. Melikidze , Krzysztof Maciesiak , Anna Skrzypczak , Andrzej Szary

Over the past decade it has become apparent that a class of `bursting pulsars' exist with the discovery of PSR J1752+2359 and PSR J1938+2213. In these pulsars, a sharp increase in the emission is observed that then tends to systematically…

Solar and Stellar Astrophysics · Physics 2014-02-10 Andrew Seymour , Duncan Lorimer , Josh Ridley

Polarization-angle density displays are given for pulsars B0809+74 and B2303+30, which exhibit no evidence of the systematic polarization-angle rotation within individual subpulses previously reported for these two stars. The ``drifting''…

We report new results from a nulling study of PSR~B0751+32 (PSR J0754+3231), observed at 1250~MHz with the Five hundred meter Aperture Spherical radio Telescope (FAST). Our analysis confirms the presence of periodic nulling in this pulsar.…

High Energy Astrophysical Phenomena · Physics 2026-04-10 W. M. Yan , N. Wang , F. F. Kou , Z. Y. Liu , J. P. Yuan , Z. G. Wen S. N. Sun , M. Y. Zou , Y. R. Wen , X. J. Chen

In this study, we report on a detailed single pulse analysis of the radio emission from the pulsar J1401$-$6357 (B1358$-$63) based on data observed with the ultrawideband low-frequency receiver on the Parkes radio telescope. In addition to…

High Energy Astrophysical Phenomena · Physics 2022-12-28 J. L. Chen , Z. G. Wen , X. F. Duan , D. L. He , N. Wang , H. G. Wang , R. Yuen , J. P. Yuan , W. M. Yan , Z. Wang , C. B. Lv , H. Wang , S. R. Cui

The phenomenon of subpulse drifting may hold the key to understanding the pulsar emission mechanism. Here, we report on new observations of PSR J0034-0721 (B0031-07), carried out with the Murchison Widefield Array at 185 MHz. We observe…

High Energy Astrophysical Phenomena · Physics 2017-03-08 S. J. McSweeney , N. D. R. Bhat , S. E. Tremblay , A. A. Deshpande , S. M. Ord

We present a single pulse study of pulsar B1944+17, whose non-random nulls dominate nearly 70% of its pulses and usually occur at mode boundaries. When not in the null state, this pulsar displays four bright modes of emission, three of…

Solar and Stellar Astrophysics · Physics 2010-07-13 Isabel M. Kloumann , Joanna M. Rankin

We report on the variation in the single-pulse emission from PSR J1900+4221 (CRAFTS 19C10) observed at frequency centered at 1.25 GHz using the Five-hundred-meter Aperture Spherical radio Telescope. The integrated pulse profile shows two…

We investigate the radio emission behaviour of PSR B0823+26, a pulsar which is known to undergo pulse nulling, using an 153-d intensive sequence of observations. The pulsar is found to exhibit both short (~min) and unusually long-term…

High Energy Astrophysical Phenomena · Physics 2015-06-11 N. J. Young , B. W. Stappers , P. Weltevrede , A. G. Lyne , M. Kramer

Several pulsars show sudden cessation of pulsed emission, which is known as nulling. The number of known nulling pulsars has not been significantly enhanced in the last decade, although the pulsar population has more than doubled following…

Solar and Stellar Astrophysics · Physics 2009-05-14 Vishal Gajjar , Bhal Chandra Joshi , M. Kramer

We present a single-pulse study of the four-component pulsar J1819+1305, whose ``null'' pulses bunch at periodic intervals of around 57 times the rotation period. The emission bursts between the null bunches exhibit characteristic…

Astrophysics · Physics 2009-06-23 Joanna M. Rankin , Geoffrey A. E. Wright

In recent years periodic amplitude modulation has emerged as a unique emission feature in the single pulse sequence of pulsars alongside periodic nulling and subpulse drifting. Despite ample evidence for the uniqueness of this phenomenon,…

High Energy Astrophysical Phenomena · Physics 2025-09-05 Rahul Basu , Dipanjan Mitra , George I. Melikidze

The phenomenon of pulsar nulling, where pulsars temporarily and stochastically cease their radio emission, is thought to be indicative of a `dying' pulsar, where radio emission ceases entirely. Here we report the discovery of a long-period…

High Energy Astrophysical Phenomena · Physics 2024-05-30 G. Grover , N. D. R. Bhat , S. McSweeney , C. P. Lee , B. W. Meyers , C. M. Tan , S. S. Kudale

We report on an analysis of the drifting subpulses of PSR B0320+39 that indicates a sudden step of ~180 degrees in subpulse phase near the centre of the pulse profile. The phase step, in combination with the attenuation of the periodic…

Astrophysics · Physics 2011-05-23 R. T. Edwards , B. W. Stappers , A. G. J. van Leeuwen

We present an analysis of the subpulse drift in PSR J1750-3503, which is characterized by abrupt transitions of drift direction. As the pulsar does not exhibit other mode changes or clear nulling, it is an ideal candidate system for…

High Energy Astrophysical Phenomena · Physics 2022-07-27 Andrzej Szary , Joeri van Leeuwen , Geoff Wright , Patrick Weltevrede , Crispin H. Agar , Caterina Tiburzi , Yogesh Maan , Michael J. Keith

New GMRT observations of the five-component pulsar B1857--26 provide detailed insight into its pulse-sequence modulation phenomena for the first time. The outer conal components exhibit a 7.4-rotation-period, longitude-stationary…

Astrophysics · Physics 2008-11-26 Dipanjan Mitra , Joanna M Rankin