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Related papers: Subpulse Drifting, Nulling and Mode changing in PS…

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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

Single-pulse studies are important to understand the pulsar emission mechanism and the noise floor in precision timing. We study total intensity and polarimetry properties of three bright millisecond pulsars - PSRs J1022+1001, J1713+0747,…

High Energy Astrophysical Phenomena · Physics 2023-01-18 N. T. Palliyaguru , B. B. P. Perera , M. A. McLaughlin , S. Oslowski , G. L. Siebert

Using new techniques based on the polarimetric fluctuation spectrum, the fluctuation behaviour of the polarization of individual pulses is examined in three pulsars that show drifting subpulses, allowing various aspects of the fluctuations…

Astrophysics · Physics 2009-11-10 R. T. Edwards

PSR B0823+26, a 0.53-s radio pulsar, displays a host of emission phenomena over timescales of seconds to (at least) hours, including nulling, subpulse drifting, and mode-changing. Studying pulsars like PSR B0823+26 provides further insight…

The research presented here examines an 8-hour observation of pulsar B1822-09,taken by the Giant Metrewave Radio Telescope. B1822-09 has been known to exhibit two stable emission modes, the B-mode, where the precursor (PC) `turns-on', and…

Solar and Stellar Astrophysics · Physics 2015-06-11 Crystal Latham , Dipanjan Mitra , Joanna Rankin

We present an analysis of approximately 200 hours of observations of the pulsars J1634$-$5107, J1717$-$4054 and J1853$+$0505, taken over the course of 14.7 yr. We show that all of these objects exhibit long term nulls and radio-emitting…

High Energy Astrophysical Phenomena · Physics 2015-06-24 N. J. Young , P. Weltevrede , B. W. Stappers , A. G. Lyne , M. Kramer

We report on radiation properties of extreme nulling pulsar J1502-5653, by analyzing the data acquired from the Parkes 64-m telescope at 1374 MHz. The radio emission from this pulsar exhibits sequences of several tens to several hundreds…

Solar and Stellar Astrophysics · Physics 2015-06-05 J. Li , A. Esamdin , R. N. Manchester , M. F. Qian , H. B. Niu

PSR J1825$-$0935 (PSR B1822$-$09) switches between radio-quiet (Q-mode) and radio-bright (B-mode) modes. The Q-mode is known to have a periodic fluctuation that modulates both the interpulse and the main pulse with the same period. Earlier…

High Energy Astrophysical Phenomena · Physics 2019-03-13 W. M. Yan , R. N. Manchester , N. Wang , J. P. Yuan , Z. G. Wen , K. J. Lee

We have observed PSR~B1534+12 (J1537+1155), a pulsar with a neutron star companion, using the Five-hundred-meter Aperture Spherical radio Telescope (FAST). We found that this pulsar shows two distinct emission states: a weak state with a…

High Energy Astrophysical Phenomena · Physics 2020-10-14 S. Q. Wang , G. Hobbs , J. B. Wang , R. Manchester , N. Wang , S. B. Zhang , Y. Feng , W. -Y. Wang , D. Li , S. Dai , K. J. Lee , S. J. Dang , L. Zhang

We have analyzed single pulses from PSR J0737-3039B, the 2.8-s pulsar in the recently discovered double pulsar system, using data taken with the Green Bank Telescope at 820 and 1400 MHz. We report the detection of features similar to…

The close correlation observed between emission state and spin-down rate change of pulsars has many implications both for the magnetospheric physics and the neutron star interior. The middle-aged pulsar PSR J0738$-$4042, which had been…

High Energy Astrophysical Phenomena · Physics 2022-11-23 S. Q. Zhou , E. Gügercinoğlu , J. P. Yuan , M. Y. Ge , C. Yu , C. M. Zhang , J. Zhang , Z. W. Feng , C. Q. Ye

Studies of subpulse variability in millisecond pulsars (MSPs) offer important constraints on their emission physics. Using the high sensitivity of FAST, we present the first identification of distinct single pulse fluctuation behaviour in…

The phenomenon of pulsar nulling, observed as the temporary inactivity of a pulsar, remains poorly understood both observationally and theoretically. Most observational studies that quantify nulling employ a variant of Ritchings (1976)'s…

High Energy Astrophysical Phenomena · Physics 2023-09-15 Akash Anumarlapudi , Joseph K. Swiggum , David L. Kaplan , Travis D. J. Fichtenbauer

PSR J1744-3922 is a binary pulsar exhibiting highly variable pulsed radio emission. We report on a statistical multi-frequency study of the pulsed radio flux variability which suggests that this phenomenon is extrinsic to the pulsar and…

The phenomenon of sub-pulse drifting is an important single-pulse phenomenon that can potentially provide important insights into the elusive radio emission mechanism in pulsars. We analyze the frequency behaviour of the single pulses of…

High Energy Astrophysical Phenomena · Physics 2023-07-26 Samuel J. McSweeney , Lisa Smith , N. D. Ramesh Bhat , Geoff Wright

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 the results of a systematic, unbiased search for subpulse modulation of 187 pulsars performed with the Westerbork Synthesis Radio Telescope (WSRT) in the Netherlands at an observing wavelength of 21 cm. Using new observations and…

Astrophysics · Physics 2009-11-11 P. Weltevrede , R. T. Edwards , B. W. Stappers

The mode switching phenomenon of PSR J0614+2229 was studied by using the archived observations at 686, 1369 and 3100 MHz with the Parkes radio telescope which have not been published before, and combining existing observations from the…

High Energy Astrophysical Phenomena · Physics 2020-02-13 Yanrong Zhang , Hongguang Wang , Xiujian Huang , Jianling Chen

Transitional millisecond pulsars are an emerging class of sources that link low-mass X-ray binaries to millisecond radio pulsars in binary systems. These pulsars alternate between a radio pulsar state and an active low-luminosity X-ray disc…

The phenomenon of profile mode switching in pulsars, where the stable average pulse profile changes to another stable state on the timescale of a pulsar's period, remains poorly understood. We sought to understand how pulsars undergo…

High Energy Astrophysical Phenomena · Physics 2019-02-13 Casey Brinkman , Dipanjan Mitra , Joanna Rankin