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Related papers: Mode Switching and Subpulse Drifting in PSR B0826-…

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We report new results obtained from multi-frequency observations of PSR B0826-34 with the Giant Metrewave Radio Telescope (GMRT). (1) We find no evidence of weak emission during the typical long null state of this pulsar, simultaneously at…

Astrophysics · Physics 2009-11-13 B. Bhattacharyya , Y. Gupta , J. Gil

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…

Solar and Stellar Astrophysics · Physics 2012-10-19 A. Esamdin , D. Abdurixit , R. N. Manchester , H. B. Niu

Aims. To make a detailed study of the nulling and subpulse drifting in PSR J1727$-$2739 for investigation of its radiation properties. Methods. The observations were carried out on 20 March, 2004 using the Parkes 64-m radio telescope, with…

High Energy Astrophysical Phenomena · Physics 2016-08-17 Z. G. Wen , N. Wang , J. P. Yuan , W. M. Yan , R. N. Manchester , R. Yuen , V. Gajjar

We report on a detailed analysis of the radio emission during the different modes of the pulsar J0826+2637 (B0823+26), observed using the Giant Meterwave Radio Telescope at 306-339 MHz observing frequencies. The pulsar profile has a…

High Energy Astrophysical Phenomena · Physics 2019-06-19 Rahul Basu , Dipanjan Mitra

We have found that there are two distinct emission modes in PSR B0809+74. Beside its normal and most common mode, the pulsar emits in a significantly different quasi-stable mode after most or possibly all nulls, occasionally for over 100…

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

We have studied the single pulse emission from two pulsars, PSR B0844-35 and PSR B1758-29, over a wide frequency range of 300-750 MHz using the uGMRT. The two pulsars have relatively wide profiles with multiple components, that are a result…

High Energy Astrophysical Phenomena · Physics 2023-10-31 Rahul Basu , Dipanjan Mitra , George I. Melikidze

The multi-drifting subpulse behaviors in PSR J2007+0910 have been studied carefully with the high sensitivity observations of the Five-hundred-meter Aperture Spherical radio Telescope (FAST) at 1250 MHz. We found that there are at least six…

High Energy Astrophysical Phenomena · Physics 2023-11-07 Xin Xu , Lunhua Shang , Qijun Zhi , Shijun Dang , Shi Dai , Jie Tian , Yan Yu , Qingying Li , Shuo Xiao , Dandan Zhang

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

PSR B0818-41 is one of the few pulsars which show multiple drift regions having well defined phase relationship. In this paper we report new results from the multifrequency GMRT observations of this pulsar. Significant linear polarization…

Astrophysics · Physics 2015-05-13 Bhaswati Bhattacharyya , Yashwant Gupta , Janusz Gil

The well known drifter PSR B0031-07 is known to exhibit drifting subpulses where the spacing between the drift bands (P_3) shows three distinct modes A, B and C corresponding to 12, 6 and 4 seconds respectively. We have investigated…

Astrophysics · Physics 2009-11-11 J. M. Smits , D. Mitra , J. Kuijpers

We report a detailed analysis of the emission behaviour of the five component, core-double cone, pulsar J2006$-$0807 (B2003$-$08). The single pulses revealed the presence of the three major phenomena of subpulse drifting, nulling and mode…

High Energy Astrophysical Phenomena · Physics 2019-05-08 Rahul Basu , Ashis Paul , Dipanjan Mitra

In this paper we analyze high time resolution single pulse data of PSR B0809+74 at 820 MHz. We compare the subpulse phase behavior, undocumented at 820 MHz, with previously published results. The subpulse period changes over time and we…

Solar and Stellar Astrophysics · Physics 2015-05-20 R. Rosen , P. Demorest

Sub-pulse drifting in pulsar radio emission is considered to be one of the most promising phenomenon for uncovering the underlying physical processes. Here we present a detailed study of such a phenomenon in observations of PSR…

High Energy Astrophysical Phenomena · Physics 2021-11-17 Parul Janagal , Manoneeta Chakraborty , N. D. Ramesh Bhat , Bhaswati Bhattacharya , Samuel J. McSweeney

Single pulse behaviour of radio pulsars is usually interpreted in terms of the ExB drift of a radio beam. It is shown that antisymmetric arrangement of the radio-bright zones can produce several types of observed single pulse phenomena: the…

High Energy Astrophysical Phenomena · Physics 2023-03-15 J. Dyks

Analyses of multiple pulse sequences of B2303+30 reveal that this pulsar has two distinct emission modes. One mode (B) follows a steady even-odd pattern and is more intense. The second mode (Q) is characteristically weak, but has…

Astrophysics · Physics 2009-11-10 Stephen L. Redman , Geoffrey A. E. Wright , Joanna M. Rankin

In this study, we report on a detailed single pulse polarimetric analysis of the radio emission from the pulsar J2321+6024 (B2319+60) observed with the Giant Metrewave Radio Telescope, over wide frequencies ranging between 300 to 500 MHz…

High Energy Astrophysical Phenomena · Physics 2022-08-15 Sk. Minhajur Rahaman , Rahul Basu , Dipanjan Mitra , George I. Melikidze

We report two phenomena detected in PSR J0344$-$0901 from two observations conducted at frequency centered at 1.25 GHz using the Five-hundred-meter Aperture Spherical radio Telescope (FAST). The first phenomenon manifests as shifting in the…

High Energy Astrophysical Phenomena · Physics 2024-02-26 H. M. Tedila , R. Yuen , N. Wang , D. Li , Z. G. Wen , W. M. Yan , J. P. Yuan , X. H. Han , P. Wang , W. W. Zhu , S. J. Dang , S. Q. Wang , J. T. Xie , Q. D. Wu , Sh. Khasanov , FAST Collaboration

We have carried out a detailed study of single pulse emission from the pulsar B2000+40 (J2002+4050), observed at 1.6 GHz frequencies using the Effelsberg radio telescope. The pulsar has three components which are not well separated, with…

High Energy Astrophysical Phenomena · Physics 2020-09-14 Rahul Basu , Wojciech Lewandowski , Jarosław Kijak

We present an analysis of the emission behaviour of PSR J1107-5907, a source known to exhibit separate modes of emission, using observations obtained over approximately 10 yr. We find that the object exhibits two distinct modes of emission;…

High Energy Astrophysical Phenomena · Physics 2015-06-19 N. J. Young , P. Weltevrede , B. W. Stappers , A. G. Lyne , M. Kramer
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