Results 111 to 120 of about 3,309 (210)

The ms pulsar - low mass X-ray binary link [PDF]

, 2016
The recent discovery of a binary millisecond pulsar in the globular cluster M28 that switched between an X-ray pulsar and a radio pulsar state demonstrated the tight link shared by millisecond pulsars and their accreting low-mass X-ray binary progenitors.
PAPITTO, ALESSANDRO
core  

A decade of transitional millisecond pulsars

, 2018
Transitional millisecond pulsars (tMSPs), which are systems that harbor a pulsar in the throes of the recycling process, have emerged as a new source class since the discovery of the first such system a decade ago.
Archibald, A., Jaodand, A., Hessels, J.W.   +2 more
core   +2 more sources

Can Slow Pulsars in Milky Way Globular Clusters Form via Partial Recycling?

The Astrophysical Journal Letters
Alongside the population of several hundred radio millisecond pulsars currently known in Milky Way globular clusters, a subset of six slowly spinning pulsars (spin periods 0.3–4 s) are also observed.
Kyle Kremer, Claire S. Ye, Craig O. Heinke, Anthony L. Piro, Scott M. Ransom, Frederic A. Rasio   +5 more
doaj   +1 more source

Discovery of 15 New Pulsars at High Galactic Latitudes with FAST

The Astrophysical Journal
We present the discovery and timing results for 15 pulsars discovered in a high-Galactic-latitude survey conducted with the Five-hundred-meter Aperture Spherical Telescope.
Xin Xu, Shi Dai, Qijun Zhi, Juntao Bai, Joanna Berteaud, Francesca Calore, Maïca Clavel, Weiwei Zhu, Di Li, Rushuang Zhao, Renxin Xu, Guojun Qiao   +11 more
doaj   +1 more source

On the aberration–retardation effects in pulsars

, 2009
The magnetospheric locations of pulsar radio emission region are not well known. The actual form of the so-called radius-to-frequency mapping should be reflected in the aberration-retardation (A/R) effects that shift and/or delay the photons depending on
Kijak, J, Krzeszowski, K., Mitra, D., Gupta, Y., Kijak, J., Acharyya, A., Mitra, D, Gupta, Y, Krzeszowski, K, Gil, J, Acharyya, A, Gil, J.   +11 more
core   +1 more source

Growth of magnetic fields in accreting millisecond pulsars

, 2013
R-modes can generate strong magnetic fields in the core of accreting millisecond neutron stars. The diffusion of these fields outside the core causes the growth of the external magnetic field and thus it affects the evolution of the spin-down rates dot{P}
CUOFANO, Carmine, PAGLIARA, Giuseppe, DRAGO, Alessandro   +2 more
core   +1 more source

'Hidden' millisecond pulsars

The Astrophysical Journal, 1991
The radiative and hydrodynamical processes occurring near the region where the pulsar wind interacts with the material outflowing from the illuminated companion star atmosphere are addressed. The emphasis is placed on the properties of a class of 'hidden' millisecond pulsars.
openaire   +1 more source

Discovery of four binary millisecond pulsars

, 1996
We present detailed parameters for four binary millisecond pulsars discovered during a survey of the southern sky with the Parkes radio telescope. Subsequent observations using the Parkes and Jodrell Bank radio telescopes have determined that the pulsars,
Stappers, B. W.; id_orcid, Lorimer, D. R., Lyne, A. G., D'Amico, N., Manchester, R. N., Camilo, F., Bailes, M., Johnston, S.   +7 more
core   +2 more sources

Observations of millisecond pulsars at 8.35 GHz

, 2003
New pulsar observations at 8.35 GHz with the newly built highly sensitive receiver of the Effelsberg 100-m Radio Telescope are reported. They resulted in the first detection of 3 millisecond pulsars J1713+0747, B1855+09 and J2145-0750 at this high ...
Wielebinski, R., Kijak, J., J. Kijak, Maron, O., O. Maron, R. Wielebinski   +5 more
core   +1 more source

Statistical Analysis of Pulsar Flux Density Distribution

The Astrophysical Journal
This study presents a comprehensive analysis of the spectral properties of 886 pulsars across a wide frequency range from 20 MHz–343.5 GHz, including a total of 86 millisecond pulsars (MSPs).
H. W. Xu, R. S. Zhao, Erbil Gugercinoglu, H. Liu, D. Li, P. Wang, C. H. Niu, C. Miao, X. Zhu, R. W. Tian, W. L. Li, S. D. Wang, Z. F. Tu, Q. J. Zhi, S. J. Dang, L. H. Shang, S. Xiao   +16 more
doaj   +1 more source