Results 91 to 100 of about 101,445 (253)

On an Autonomous Pulsar Observation–Based Timekeeping Method for Deep Space

International Journal of Aerospace Engineering, Volume 2025, Issue 1, 2025.
To provide autonomous and accurate time service for deep space missions, a pulsar observation–based timekeeping method is documented in this paper, which utilizes pulsars as the time information source. Firstly, the pulsar observation noise is remodeled as the combination of the Gaussian noise and colored noise, and the detailed expression of the ...
Shibin Song, Xiaowei Jin, Haixia Wang, Giovanni Palmerini   +3 more
wiley   +1 more source

Gamma-ray Burst Afterglow with Continuous Energy Injection: Signature of a Highly-Magnetized Millisecond Pulsar

, 2001
We investigate the consequences of a continuously injecting central engine on the gamma-ray burst afterglow emission, focusing more specifically on a highly-magnetized millisecond pulsar engine.
Bing Zhang, Dai Z. G., Masetti N., Peter Mészáros, Spruit H. C., Thompson C.   +5 more
core   +1 more source

Broadband X-ray spectra and timing of the accreting millisecond pulsar Swift J1756.9–2508 during its 2018 and 2019 outbursts [PDF]

, 2021
Z. S. Li, L. Kuiper, M. Falanga, J. Poutanen, Sergey S. Tsygankov, D K Galloway, E. Bozzo, Y. Y. Pan, Y. Huang, SN Zhang, S Zhang, Z. S. Li, M. Falanga, J. Poutanen, Sergey S. Tsygankov, D K Galloway, E. Bozzo, Y. Y. Pan, Y. Huang, SN Zhang, S Zhang   +20 more
openalex   +1 more source

PSR J1024–0719: A MILLISECOND PULSAR IN AN UNUSUAL LONG-PERIOD ORBIT [PDF]

, 2016
PSR J1024–0719 is a millisecond pulsar that was long thought to be isolated. However, puzzling results concerning its velocity, distance, and low rotational period derivative have led to a reexamination of its properties.
D. Kaplan, T. Kupfer, D. Nice, A. Irrgang, U. Heber, Z. Arzoumanian, E. Beklen, K. Crowter, M. DeCesar, P. Demorest, T. Dolch, J. Ellis, R. Ferdman, E. Ferrara, E. Fonseca, P. Gentile, G. Jones, Megan L. Jones, S. Kreuzer, M. Lam, L. Levin, D. Lorimer, R. Lynch, M. Mclaughlin, A. Miller, C. Ng, T. Pennucci, T. Prince, S. Ransom, P. Ray, R. Spiewak, I. Stairs, K. Stovall, J. Swiggum, Weiwei Zhu   +34 more
semanticscholar   +1 more source

Search for Short‐Duration Transient Gravitational Waves Emitted by Neutron Star Glitches

Annalen der Physik, Volume 536, Issue 2, February 2024.
The observation rate of pulsar glitches is limited by their electromagnetic observations. There could be a population of the isolated neutron stars in the galaxy for which there is no electromagnetic observations, but they can produce gravitational waves. The all‐sky search for gravitational waves provides better localization of the source sky position
Dixeena Lopez, the LIGO, Virgo, and KAGRA collaborations   +3 more
wiley   +1 more source

Identifying Companions in Pulsar Binary Systems via Gaia Data

Universe
In the optical band, very few pulsars can be directly detected, but some of the pulsar binary companions can be observed. This study leverages high-precision astrometric data from Gaia Data Release 3 (DR3) to identify pulsar companions in binary systems.
Yueqi Song, Li Guo, Zhen Yan, Qiqi Wu, Guangli Wang, Ying Wang   +5 more
doaj   +1 more source

The NANOGrav 12.5 yr Data Set: Polarimetry and Faraday Rotation Measures from Observations of Millisecond Pulsars with the Green Bank Telescope

The Astrophysical Journal, 2022
In this work, we present polarization profiles for 23 millisecond pulsars observed at 820 and 1500 MHz with the Green Bank Telescope as part of the NANOGrav pulsar timing array.
H. M. Wahl, M. A. McLaughlin, P. A. Gentile, M. L. Jones, R. Spiewak, Z. Arzoumanian, K. Crowter, P. B. Demorest, M. E. DeCesar, T. Dolch, J. A. Ellis, R. D. Ferdman, E. C. Ferrara, E. Fonseca, N. Garver-Daniels, G. Jones, M. T. Lam, L. Levin, N. Lewandowska, D. R. Lorimer, R. S. Lynch, D. R. Madison, C. Ng, D. J. Nice, T. T. Pennucci, S. M. Ransom, P. Ray, I. H. Stairs, K. Stovall, J. K. Swiggum, W. W. Zhu   +30 more
doaj   +1 more source

Twenty Years of Searching for (and Finding) Globular Cluster Pulsars

, 2007
Globular clusters produce orders of magnitude more millisecond pulsars per unit mass than the Galactic disk. Since the first cluster pulsar was uncovered twenty years ago, at least 138 have been identified - most of which are binary millisecond pulsars ...
A. Cumming, C. Bassa, Scott M. Ransom, V. M. Kaspi, Z. Wang   +4 more
core   +1 more source

DISCOVERY OF A REDBACK MILLISECOND PULSAR CANDIDATE: 3FGL J0212.1+5320 [PDF]

, 2016
We present a multiwavelength study of the unidentified Fermi object, 3FGL J0212.1+5320. Within the 95% error ellipse, Chandra detects a bright X-ray source (i.e., erg cm−2 s−1) that has a low-mass optical counterpart ( and K).
Kwan-Lok Li, A. Kong, X. Hou, J. Mao, J. Strader, L. Chomiuk, E. Tremou   +6 more
semanticscholar   +1 more source

Heavy Elements and Electromagnetic Transients from Neutron Star Mergers

Annalen der Physik, Volume 536, Issue 2, February 2024.
Astro‐(physics) has made major leaps forward through the combined information provided by both gravitational waves and electromagnetic emission from the first detected neutron star merger event. This review provides an up‐to‐date overview of today's understanding of neutron star mergers and their electromagnetic emission and it discusses possible ...
Stephan Rosswog, Oleg Korobkin
wiley   +1 more source