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1
Published in 2017 at "Astronomische Nachrichten"
DOI: 10.1002/asna.201713436
Abstract: The low braking-index pulsar PSR J1734$-$3333 could be born with superhigh internal magnetic fields $B_{\rm in}\sim10^{15}-10^{16}$ G, and undergo a supercritical accretion soon after its formation in a supernova explosion. The buried multipole magnetic fields…
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Keywords:
index;
index pulsar;
pulsar;
field ... See more keywords
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1
Published in 2018 at "Acta Astronautica"
DOI: 10.1016/j.actaastro.2017.11.014
Abstract: Abstract This paper develops a timing solution for the X-ray pulsar timing model without the use of the initial radio model parameters. First, we address the problem of phase ambiguities for the pre-fit residuals in…
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Keywords:
pulsar;
radio;
model;
ray pulsar ... See more keywords
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1
Published in 2020 at "Acta Astronautica"
DOI: 10.1016/j.actaastro.2019.10.016
Abstract: Abstract Existing methods for simulating pulsar signals at a spacecraft are inapplicable for large flux or high frequency because of their low efficiency, hindering research on X-ray pulsar-based navigation. To solve the problem, we propose…
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Keywords:
pulsar;
pulsar signals;
fast simulation;
ray pulsar ... See more keywords
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3
Published in 2023 at "Publications of the Astronomical Society of Australia"
DOI: 10.1017/pasa.2023.18
Abstract: Abstract In Paper I, we presented an overview of the Southern-sky MWA Rapid Two-metre (SMART) survey, including the survey design and search pipeline. While the combination of MWA’s large field-of-view and the voltage capture system…
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Keywords:
pulsar discoveries;
sky mwa;
survey;
pulsar ... See more keywords
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0
Published in 2024 at "Publications of the Astronomical Society of Australia"
DOI: 10.1017/pasa.2024.64
Abstract: Abstract PSR J0837 $-$ 2454 is a young 629 ms radio pulsar whose uncertain distance has important implications. A large distance would place the pulsar far out of the Galactic plane and suggest it is…
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Keywords:
pulsar;
direct urca;
psr j0837;
j0837 2454 ... See more keywords
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Published in 2024 at "Publications of the Astronomical Society of Australia"
DOI: 10.1017/pasa.2024.96
Abstract: Abstract The spin-down law of pulsars is generally perturbed by two types of timing irregularities: glitches and timing noise. Glitches are sudden changes in the rotational frequency of pulsars, while timing noise is a discernible…
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Keywords:
glitch;
pulsar;
analysis;
timing noise ... See more keywords
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0
Published in 2017 at "Nature Astronomy"
DOI: 10.1038/s41550-017-0266-2
Abstract: Millisecond pulsars are neutron stars that attain their very fast rotation during a 108–109-yr-long phase of disk accretion of matter from a low-mass companion star1,2. They can be detected as accretion-powered millisecond X-ray pulsars if…
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Keywords:
pulsar;
accretion;
millisecond;
optical pulsations ... See more keywords
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Published in 2024 at "Nature Astronomy"
DOI: 10.1038/s41550-025-02534-6
Abstract: The ionized interstellar medium contains astronomical-unit-scale (and below) structures that scatter radio waves from pulsars, resulting in scintillation. Power spectral analysis of scintillation often shows parabolic arcs, with curvatures that encode the locations and kinematics…
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Keywords:
pulsar;
local bubble;
millisecond pulsar;
j0437 4715 ... See more keywords
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Published in 2025 at "Scientific Reports"
DOI: 10.1038/s41598-025-25591-3
Abstract: In the surrounding orbits, the position error of the spacecraft causes the distortion of the accumulative pulsar profile. Through theoretical analysis, a non-sensitive direction exists in three-dimensional space. Specifically, the initial position error in the…
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Keywords:
pulsar;
non sensitive;
dimensional positioning;
two dimensional ... See more keywords
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Published in 2020 at "Astronomy and Astrophysics"
DOI: 10.1051/0004-6361/201936525
Abstract: Context. The Argentine Institute of Radio astronomy (IAR) is equipped with two single-dish 30 m radio antennas capable of performing daily observations of pulsars and radio transients in the southern hemisphere at 1.4 GHz. Aims:…
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Keywords:
radio astronomy;
institute radio;
argentine institute;
pulsar ... See more keywords
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1
Published in 2020 at "Astronomy and Astrophysics"
DOI: 10.1051/0004-6361/202037873
Abstract: In this work, we study the X-ray bow-shock nebula powered by the mature pulsar PSR B1929+10 using data from XMM-Newton, with an effective exposure of $\sim$ 300 ks, offering the deepest investigation of this system…
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Keywords:
nebula;
bow shock;
psr b1929;
pulsar ... See more keywords