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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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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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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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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 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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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
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1
Published in 2022 at "Research in Astronomy and Astrophysics"
DOI: 10.1088/1674-4527/ac3e5e
Abstract: 4FGL J0935.5+0901, a γ-ray source recently identified as a candidate redback-type millisecond pulsar (MSP) binary, shows an interesting feature of having double-peaked emission lines in its optical spectrum. This feature would further suggest the source…
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Keywords:
millisecond pulsar;
pulsar;
j0935 0901;
4fgl j0935 ... See more keywords
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Published in 2023 at "Research in Astronomy and Astrophysics"
DOI: 10.1088/1674-4527/acd89d
Abstract: We report the discovery of PSR J1909+0122 by the Five-hundred-meter Aperture Spherical radio Telescope (FAST) as part of the Commensal Radio Astronomy FAST Survey (CRAFTS). PSR J1909+0122 has a spin period of 1.257 seconds, a…
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Keywords:
j1909;
j1909 0122;
pulsar;
astronomy ... See more keywords
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1
Published in 2020 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/staa2703
Abstract: eHWC J2019+368 is one of the sources emitting $\gamma$-rays with energies higher than 100 TeV based on the recent measurement with the High Altitude Water Cherenkov Observatory (HAWC), and the origin is still in debate.…
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Keywords:
pulsar;
ehwc j2019;
tev;
j2019 368 ... See more keywords
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1
Published in 2020 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/staa287
Abstract: We report results of XMM–Newton observations of a γ-ray pulsar J0633+0632 and its wind nebula. We reveal, for the first time, pulsations of the pulsar X-ray emission with a single sinusoidal pulse profile and a…
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Keywords:
emission;
ray pulsar;
pulsar;
newton observations ... See more keywords