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相关论文: High Energy Radiation from Spider Pulsars

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In this paper, we study compact binary millisecond pulsars with low- and very low-mass companion stars (spiders) in the Galactic field, using data from the latest Gaia data release (DR3). We infer the parallax distances of the optical…

高能天体物理现象 · 物理学 2023-08-16 Karri I. I. Koljonen , Manuel Linares

We have performed a systematic study of the rotational, orbital and X-ray properties of millisecond pulsars (MSPs) in globular clusters (GCs) and compared their nature with those of the MSPs in the Galactic field (GF). We found that GC MSPs…

高能天体物理现象 · 物理学 2023-03-08 Jongsu Lee , C. Y. Hui , J. Takata , A. K. H. Kong , Pak-Hin Thomas Tam , Kwan-Lok Li , K. S. Cheng

We report the discovery of two Black Widow millisecond pulsars in the globular cluster M28 with the MeerKAT telescope. PSR J1824$-$2452M (M28M) is a 4.78-ms pulsar in a $5.82\,$hour orbit and PSR J1824$-$2452N (M28N) is a 3.35-ms pulsar in…

We present the timing solution for the 5.31-ms spider millisecond pulsar (MSP) J1242-4712, discovered with the GMRT. PSR J1242-4712 orbits a companion of minimum mass 0.08 M$_{\odot}$ with an orbital period of 7.7 hrs and occupies a…

Redback millisecond pulsars (hereafter redbacks) are a sub-population of eclipsing millisecond pulsars in close binaries. The formation processes of these systems are not clear. The three pulsars showing transitions between rotation- and…

高能天体物理现象 · 物理学 2015-10-26 Kun Jia , Xiang-Dong Li

We have monitored a large sample of millisecond pulsars using the 100-m Effelsberg radio telescope in order to compare their radio emission properties to the slowly rotating population. With some notable exceptions, our findings suggest…

天体物理学 · 物理学 2009-10-30 M. Kramer , K. M. Xilouris , D. Lorimer , O. Doroshenko , A. Jessner , R. Wielebinski , A. Wolszczan , F. Camilo

The 2nd Fermi-LAT pulsar catalog includes 117 gamma-ray pulsars, of which roughly one third are millisecond pulsars (MSPs) while the remaining two thirds split evenly into young radio-loud and radio-quiet pulsars. Although this large…

高能天体物理现象 · 物理学 2015-06-12 Matthew Kerr , the Fermi-LAT Collaboration

4FGL J0935.5+0901, a $\gamma$-ray source recently identified as a candidate redback-type millisecond pulsar binary (MSP), shows an interesting feature of having double-peaked emission lines in its optical spectrum. The feature would further…

高能天体物理现象 · 物理学 2022-02-16 Dong Zheng , Zhong-Xiang Wang , Yi Xing , Jithesh Vadakkumthani

Binary millisecond pulsars (MSPs) provide several opportunities for research of fundamental physics. However, finding them can be challenging. Several subdwarf B (sdB) binary systems with possible neutron star companions have been…

高能天体物理现象 · 物理学 2020-01-22 L. C. Oostrum , J. van Leeuwen , Y. Maan , T. Coenen , C. H. Ishwara-Chandra

We compare the spectral properties of the millisecond and slow pulsars detected in the Parkes 70 cm survey. The mean spectral index for the millisecond pulsars (MSPs) is -1.9 +/- 0.1 whereas the mean spectral index for the slow pulsars is a…

天体物理学 · 物理学 2009-10-30 M. Toscano , M. Bailes , R. N. Manchester , J. S. Sandhu

Several redback and black widow millisecond pulsar binaries have episodes of flaring in X-rays and optical. We initially detected such behavior from the Fermi selected redback candidate 1FGL J0523.5$-$2529 during optical time-series…

高能天体物理现象 · 物理学 2022-08-31 Jules P. Halpern , Karen I. Perez , Slavko Bogdanov

Millisecond pulsars (MSPs) are prolific GeV $\gamma\text{-ray}$ emitters, and nearly 80\% of Fermi-LAT MSPs reside in compact binaries. We demonstrate that the companions in these compact MSPs binaries are also 511 keV annihilation line…

高能天体物理现象 · 物理学 2025-09-05 Zachary Metzler , Zorawar Wadiasingh

Pair cascades from millisecond pulsars (MSPs) may be a primary source of Galactic electrons and positrons that contribute to the increase in positron flux above 10 GeV as observed by PAMELA and AMS-02. The Fermi Large Area Telescope (LAT)…

高能天体物理现象 · 物理学 2015-08-20 Christo Venter , Andreas Kopp , Alice K Harding , Peter L Gonthier , Ingo Buesching

We report our analysis of the Fermi Large Area Telescope data for 39 millisecond pulsars (MSPs) listed in the second $\gamma$-ray pulsar catalog. Spectra of the pulsars are obtained. We fit the spectra with a function of a power law with…

高能天体物理现象 · 物理学 2016-11-09 Yi Xing , Zhongxiang Wang

The number of millisecond pulsars (MSPs) observed in Milky Way globular clusters has increased explosively in recent years, but the underlying population is still uncertain due to observational biases. We use state-of-the-art $N$-body…

高能天体物理现象 · 物理学 2022-12-07 Claire S. Ye , Giacomo Fragione

Eclipsing pulsar binaries and binaries with a high mass companion are ideal systems for studying and understanding the properties of plasma in magneto-ionic environments. In this work, the first paper of a series, we present MeerKAT…

Millisecond pulsars represent an evolutionarily distinct group among rotation-powered pulsars. Outside the radio band, the soft X-ray range ($\sim 0.1$--10 keV) is most suitable for studying radiative mechanisms operating in these…

天体物理学 · 物理学 2008-11-26 Vyacheslav E. Zavlin

The X-ray and gamma-ray spectrum of rotation-powered millisecond pulsars is investigated in a model for acceleration and pair cascades on open field lines above the polar caps. Although these pulsars have low surface magnetic fields, their…

天体物理学 · 物理学 2016-08-30 Alice K. Harding , Vladimir V. Usov , Alex G. Muslimov

'Spider' binary systems - black widow and redback compact binaries differentiated by their companion's mass and nature - are an important type of pulsar system exhibiting a rich empirical phenomenology, including radio eclipses, optical…

高能天体物理现象 · 物理学 2026-02-12 Christo Venter , Andreas Kopp , Zorawar Wadiasingh , Alice K Harding , M Baring

Observations by the Fermi Large Area Telescope of gamma-ray millisecond pulsar light curves imply copious pair production in their magnetospheres, and not exclusively in those of younger pulsars. Such pair cascades may be a primary source…

高能天体物理现象 · 物理学 2015-07-15 C. Venter , A. Kopp , A. K. Harding , P. L. Gonthier , I. Büsching