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相关论文: Subpulse Drifting, Nulling and Mode changing in PS…

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We report on a detailed study of the mode switching in pulsar J1326$-$6700 by analyzing the data acquired from the Parkes 64 m radio telescope at 1369 MHz. During the abnormal mode, the emission at the central and trailing components…

高能天体物理现象 · 物理学 2020-12-02 Z. G. Wen , W. M. Yan , J. P. Yuan , H. G. Wang , J. L. Chen , M. Mijit , R. Yuen , N. Wang , Z. Y. Tu , S. J. Dang

The radio millisecond pulsar PSR J1023+0038 exhibits complex timing and eclipse behavior. Here we analyze four years' worth of radio monitoring observations of this object. We obtain a long-term timing solution, albeit with large residual…

高能天体物理现象 · 物理学 2013-11-21 Anne M. Archibald , Victoria M. Kaspi , Jason W. T. Hessels , Ben Stappers , Gemma Janssen , Andrew Lyne

We present a study of timing properties of the accreting pulsar 2S 1417-624 observed during its 2018 outburst, based on Swift/BAT, Fermi/GBM, Insight-HXMT and NICER observations. We report a dramatic change of the pulse profiles with…

A novel scheme has been developed to show that the observed phase behaviour associated with subpulse drifting from two pulsars, J1034$-$3224 and J1720$-$2933, can be used to obtain the magnetic field configuration in the partially screened…

高能天体物理现象 · 物理学 2023-05-24 Rahul Basu , Dipanjan Mitra , George I. Melikidze

Transitional millisecond pulsars are systems that alternate between an accreting low-mass X-ray binary (LMXB) state, and a non-accreting radio pulsar state. When at the LMXB state, their X-ray and optical light curves show rapid flares and…

高能天体物理现象 · 物理学 2017-12-27 Pasi Hakala , Jari J. E. Kajava

The pulsar B1822-09 (J1825-0935) experienced a series of five unusual slow glitches over the 1995-2004 interval. The results of further study of this unusual glitch phenomenon are presented. It is also reported the detection a new glitch of…

天体物理学 · 物理学 2008-11-26 Tatiana V. Shabanova

We present evidence that the integrated profiles of some millisecond pulsars exhibit severe changes that are inconsistent with the moding phenomenon as known from slowly rotating pulsars. We study these profile instabilities in particular…

天体物理学 · 物理学 2009-10-31 M. Kramer , K. M. Xilouris , F. Camilo , D. J. Nice , D. C. Backer , C. Lange , D. R. Lorimer , O. Doroshenko , S. Sallmen

We report a detailed multi-frequency study of significant instabilities observed in the average pulse profile of the 16-millisecond pulsar PSR J1022+1001. These unusual profile variations which are seen as a function of time and of radio…

天体物理学 · 物理学 2009-11-10 R. Ramachandran , M. Kramer

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…

太阳与恒星天体物理 · 物理学 2015-05-20 R. Rosen , P. Demorest

We present a comprehensive study of the rotational and emission properties of PSR J0738$-$4042 using a combination of observations taken by the Deep Space Network, Hartebeesthoek, Parkes (Murriyang) and Molonglo observatories between 1972…

Transitional millisecond pulsars provide a unique set of observational data for understanding accretion at low rates onto magnetized neutron stars. In particular, PSR~J1023+0038 exhibits a remarkable bimodality of the X-ray luminosity (low…

高能天体物理现象 · 物理学 2019-11-06 Alexandra Veledina , Joonas Nättilä , Andrei M. Beloborodov

Timing analysis of PSR J1705$-$1906 using data from Nanshan 25-m and Parkes 64-m radio telescopes, which span over fourteen years, shows that the pulsar exhibits significant proper motion, and rotation instability. We updated the astrometry…

高能天体物理现象 · 物理学 2018-10-23 Y. L. Liu , J. P. Yuan , J. B. Wang , X. W. Liu , N. Wang , R. Yuen

We study the bi-drifting pulsar B1839-04, where the observed subpulse drift direction in the two leading pulse components is opposite from that in the two trailing components. Such diametrically opposed apparent motions challenge our…

高能天体物理现象 · 物理学 2020-07-01 Andrzej Szary , Joeri van Leeuwen , Patrick Weltevrede , Yogesh Maan

Mildly recycled pulsars are neutron stars partially spun up through relatively short mass-transfer phases, typically with massive carbon-oxygen (CO) or oxygen-neon-magnesium (ONeMg) white dwarf companions. PSR J2338+4818, a mildly recycled…

Most millisecond pulsars, like essentially all other radio pulsars, show timing errors well in excess of what is expected from additive radiometer noise alone. We show that changes in amplitude, shape and pulse phase for the millisecond…

太阳与恒星天体物理 · 物理学 2015-06-11 Ryan M. Shannon , James M. Cordes

The longitude separation between adjacent drifting subpulses, $P_2$, is roughly constant for many pulsars. It was then perplexing when pulsar B0809+74 was found to exhibit substantial variations in this measure, both with wavelength and…

天体物理学 · 物理学 2009-11-10 Joanna M. Rankin , R. Ramachandran , Svetlana A. Suleymanova

PSR B1828-11 is a young pulsar once thought to be undergoing free precession and recently found instead to be switching magnetospheric states in tandem with spin-down changes. Here we show the two extreme states of the mode-changing found…

高能天体物理现象 · 物理学 2019-03-06 I. H. Stairs , A. G. Lyne , M. Kramer , B. W. Stappers , J. van Leeuwen , A. Tung , R. N Manchester , G. B. Hobbs , D. R. Lorimer , A. Melatos

We report the independent discovery of PSR J0027-1956 with the Murchison Widefield Array (MWA) in the ongoing Southern-sky MWA Rapid Two-meter (SMART) pulsar survey. J0027-1956 has a period of ~1.306 s, a dispersion measure (DM) of ~20.869…

For many years it has been considered puzzling how pulsar radio emission, supposedly created by a circulating carousel of sub-beams, can produce the driftbands demonstrated by PSR J0815+09, and more recently PSR B1839-04, which…

高能天体物理现象 · 物理学 2016-11-23 Geoff Wright , Patrick Weltevrede

We present the statistical 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 (Weltevrede et…

天体物理学 · 物理学 2007-05-23 P. Weltevrede , R. T. Edwards , B. W. Stappers