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相关论文: Discovery of state transition behaviors in PSR J11…

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PSR J2021+4026 is a radio-quiet gamma-ray pulsar and the first pulsar that shows state change of the gamma-ray emission and spin-down rate. The state change of PSR J2021+4026 was first observed at 2011 October, at which the pulsar changes…

高能天体物理现象 · 物理学 2020-02-19 J. Takata , H. H. Wang , L. C. C. Lin , C. -P. Hu , C. Y. Hui , A. K. H. Kong , P. H. T. Tam , K. L. Li , K. S. Cheng

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)…

天体物理学 · 物理学 2009-11-07 S. M. Ord , R. Edwards , M. Bailes

The young pulsar PSR B1828-11 has long been known to show correlated shape and spin-down changes with timescales of roughly 500 and 250 days, perhaps associated with large-scale magnetospheric switching. Here we present multi-hour…

高能天体物理现象 · 物理学 2019-03-13 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 study the spin-down properties of PSR B0919+06 based on almost 30 years of radio observations. We confirm that the time derivative of the rotational frequency $\dot \nu$ is modulated quasi-periodically and show that it exhibits a…

太阳与恒星天体物理 · 物理学 2015-06-23 B. B. P. Perera , B. W. Stappers , P. Weltevrede , A. G. Lyne , C. G. Bassa

Using a highly accurate numerical code, we study the spin down of rotating relativistic stars, undergoing a quark deconfinement phase transition. Such phase transitions have been suggested to yield an observable signal in the braking index…

天体物理学 · 物理学 2009-11-07 N. K. Spyrou , N. Stergioulas

Transitional millisecond pulsars (tMSPs) switch, on roughly multi-year timescales, between rotation-powered radio millisecond pulsar (RMSP) and accretion-powered low-mass X-ray binary (LMXB) states. The tMSPs have raised several questions…

We present an analysis of 4 nulling pulsars with the Five-hundred-meter Aperture Spherical radio Telescope (FAST). For PSR J1649+2533, our results suggest mode changing rather than subpulse drifting as previously reported at lower…

高能天体物理现象 · 物理学 2025-11-07 Jingbo Wang , Jintao Xie , Jing Zou , Jianfei Tang

We study the spin-down changes of PSR B1859$+$07 over a period of more than 28 years of radio observation. We identify that the time derivative of the rotational frequency ($\nu$) varies quasi-periodically with a period of $\sim$350 days,…

太阳与恒星天体物理 · 物理学 2015-11-18 B. B. P. Perera , B. W. Stappers , P. Weltevrede , A. G. Lyne , J. M. Rankin

PSR J0742-2822 exhibits two distinct emission states that are identified by discrete changes in the observed pulse profile. These changes have previously been shown to correlate with changes in the derivative of the pulse frequency. In this…

太阳与恒星天体物理 · 物理学 2015-06-15 M. J. Keith , R. M. Shannon , S. Johnston

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

PSR J2021+4026 is a remarkable $\gamma$-ray pulsar exhibiting repeated transitions between high $\gamma$-ray flux (HGF) and low $\gamma$-ray flux (LGF) states. With 17-yr Fermi-LAT monitoring, we reveal persistent secular evolution and…

Measuring a pulsar's rotational evolution is crucial to understanding the nature of the pulsar. Here we provide updated timing models for the rotational evolution of six pulsars, five of which are rotation phase-connected using primarily…

The way pulsars spin down is not understood in detail, but a number of possible physical mechanisms produce a spin-down rate that scales as a power of the rotation rate ($\dot\nu\propto-\nu^n$), with the power-law index $n$ called the…

PSR B0540-69 has braking index measurement in its persistent state: n=2.129 \pm 0.012. Recently, it is reported to have spin-down state changes: a suddenly 36 % increase in the spin-down rate. Combining the persistent state braking index…

高能天体物理现象 · 物理学 2016-05-25 F. F. Kou , Z. W. Ou , H. Tong

In this work, we report the discovery and characterization of PSR J1411+2551, a new binary pulsar discovered in the Arecibo 327 MHz Drift Pulsar Survey. Our timing observations of the radio pulsar in the system span a period of about 2.5…

高能天体物理现象 · 物理学 2018-04-03 J. G. Martinez , K. Stovall , P. C. C. Freire , J. S. Deneva , T. M. Tauris , A. Ridolfi , N. Wex , F. A. Jenet , M. A. McLaughlin , M. Bagchi

PSR J1023+0038 (J1023) is a binary system hosting a neutron star and a low mass companion. J1023 is the best studied transitional pulsar, alternating a faint eclipsing millisecond radio pulsar state to a brighter X-ray active state. At…

高能天体物理现象 · 物理学 2017-09-27 S. Campana , F. Coti Zelati , A. Papitto , N. Rea , D. F. Torres , M. C. Baglio , P. D'Avanzo

We investigate the high energy emission activities of two bright gamma-ray pulsars, PSR~J2021+4026 and Vela. For PSR~J2021+4026, the state changes in the gamma-ray flux and spin-down rate have been observed. We report that the long-term…

高能天体物理现象 · 物理学 2024-01-19 H. -H. Wang , J. Takata , L. C. -C. Lin , P. -H. T. Tam

Considering about seven years of Fermi-Large Area Telescope (LAT) data, we present a systematic search for variability possibly related to transitions between states in redbacks and black widow systems. Transitions are characterized by…

高能天体物理现象 · 物理学 2017-02-15 Diego F. Torres , Long Ji , Jian Li , Alessandro Papitto , Nanda Rea , Emma de Ona Wilhelmi , Shu Zhang

We report on radio and X-ray observations of PSR 1832+0029, a 533-ms radio pulsar discovered in the Parkes Multibeam Pulsar Survey. From radio observations taken with the Parkes, Lovell and Arecibo telescopes, we show that this pulsar…

高能天体物理现象 · 物理学 2012-10-11 D. R. Lorimer , A. G. Lyne , M. A. McLaughlin , G. G. Pavlov , C. Chang

PSR J2032+4127 is a gamma-ray and radio-emitting pulsar which has been regarded as a young luminous isolated neutron star. However, its recent spin-down rate has extraordinarily increased by a factor of two. We present evidence that this is…

高能天体物理现象 · 物理学 2015-02-06 Andrew Lyne , Ben Stappers , Michael Keith , Paul Ray , Matthew Kerr , Fernando Camilo , Tyrel Johnson
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