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Extremely low-mass white dwarfs (ELM WDs) are helium-core white dwarfs with masses less than 0.3 $M_{\odot}$. Short-period ELM WD binaries that exhibit ellipsoidal variations may harbor heavier companions, either massive white dwarfs or…

太阳与恒星天体物理 · 物理学 2024-12-24 W. J. Huang , Pak-Hin Thomas Tam , L. L. Ren , J. M. Lin

The Low-Frequency Array radio telescope discovered the $707$ Hz binary millisecond pulsar (MSP) J0952$-$0607 in a targeted radio pulsation search of an unidentified $\textit{Fermi}$ gamma-ray source. This source shows a weak energy flux of…

Black widows (BWs) are millisecond pulsars ablating their companion stars. The out-flowing material from the companion can block the radio emission of the pulsar, resulting in eclipses. In this paper, we construct a model for the radio…

高能天体物理现象 · 物理学 2023-10-13 Ze-Xin Du , Yun-Wei Yu , A-Ming Chen , Shuang-Qiang Wang , Xia Zhou , Xiao-Ping Zheng

We report the discovery of 1.97 ms period gamma-ray pulsations from the 75 minute orbital-period binary pulsar now named PSR J1653-0158. The associated Fermi Large Area Telescope gamma-ray source 4FGL J1653.6-0158 has long been expected to…

Microstructure emission, involving short time scale, often quasi-periodic, intensity fluctuations in subpulse emission, is well known in normal period pulsars. In this letter, we present the first detections of quasi-periodic microstructure…

高能天体物理现象 · 物理学 2016-12-06 Kishalay De , Yashwant Gupta , Prateek Sharma

Binary radio pulsar system J0737-3039 provides an exceptional opportunity to study innermost structure of pulsar magnetospheres due to very tight orbit, favorable directions of pulsars' rotation and magnetic axes and extremely fortuitous…

天体物理学 · 物理学 2016-08-30 Maxim Lyutikov

We report the detection of 48 millisecond pulsars (MSPs) out of 75 observed thus far using the LOFAR in the frequency range 110-188 MHz. We have also detected three MSPs out of nine observed in the frequency range 38-77 MHz. This is the…

We consider the population of black widow pulsars (BWPs). The large majority of these are members of globular clusters. For minimum companion masses < 0.1 Msun, adiabatic evolution and consequent mass loss under gravitational radiation…

天体物理学 · 物理学 2009-11-10 A. R. King , M. E. Beer , D. J. Rolfe , K. Schenker , J. M. Skipp

Time-domain analysis of an archival XMM-Newton observation unveiled a very unusual variability pattern in the soft X-ray emission of PSR J1311-3430, a black widow millisecond pulsar in a tight binary (P_B=93.8 min) with a very low-mass…

高能天体物理现象 · 物理学 2022-11-16 Andrea De Luca , Martino Marelli , Sandro Mereghetti , Ruben Salvaterra , Roberto Mignani , Andrea Belfiore

PSR J1903+0327 is a mili-second pulsar with a mass of 1.67 M_{\odot} in a highly eccentric orbit (e=0.44) around a main-sequence star. This unique system cannot be reconciled with current observations where milli-second pulsars are…

高能天体物理现象 · 物理学 2015-05-30 Juthika Khargharia , John T. Stocke , Cynthia S. Froning , Achamveedu Gopakumar , Bhal Chandra Joshi

We report the results of a blind pulsar survey carried out with the Giant Metrewave Radio Telescope (GMRT) at 325 MHz. The survey covered about 10\% of the region between Galactic longitude 45$^{\circ} < l <$ 135$^{\circ}$ and Galactic…

We report the discovery of the millisecond pulsar PSR J2043+1711 in a search of a Fermi Large Area Telescope (LAT) source with no known associations, with the Nancay Radio Telescope. The new pulsar, confirmed with the Green Bank Telescope,…

Context. PSR J0312$-$0921 and PSR J1627$+$3219 are black widow pulsars with orbital periods of 2.34 and 3.98 hours. They were recently detected in the radio and $\gamma$-rays. Aims. Our goals are to estimate the fundamental parameters of…

高能天体物理现象 · 物理学 2025-11-14 A. V. Bobakov , A. Kirichenko , S. V. Zharikov , D. A. Zyuzin , A. V. Karpova , Yu. A. Shibanov , T. Begari

With recent advances in the sensitivity of radio surveys of the Galactic disk, the number of millisecond pulsars (MSPs) has increased substantially in recent years such that it is now possible to study their demographic properties in more…

高能天体物理现象 · 物理学 2022-03-14 Kshitij Aggarwal , Duncan. R. Lorimer

We present the discovery and timing solutions of four millisecond pulsars (MSPs) discovered in the Arecibo 327 MHz Drift-Scan Pulsar Survey. Three of these pulsars are in binary systems, consisting of a redback (PSR J2055+1545), a black…

The recent detection of circularly polarized, long-duration (>8 hr) low-frequency (~150 MHz) radio emission from the M4.5 dwarf GJ 1151 has been interpreted as arising from a star-planet interaction via the electron cyclotron maser…

We used photometric data from the WASP (Wide-Angle Search for Planets) survey to explore the possibility of detecting eclipses and transit signals of brown dwarfs, gas giants and terrestrial companions in close orbit around white dwarfs. We…

地球与行星天体物理 · 物理学 2015-05-20 F. Faedi , R. G. West , M. R. Burleigh , M. R. Goad , L. Hebb

We present a comprehensive census of X-ray millisecond pulsars (MSPs) in 29 Galactic globular clusters (GCs), including 68 MSPs with confirmed X-ray luminosities and 107 MSPs with X-ray upper limits. We compile previous X-ray studies of GC…

高能天体物理现象 · 物理学 2022-03-02 Jiaqi Zhao , Craig O. Heinke

Targeted searches for pulsars based on their counterparts in radio images have resulted in the discovery of interesting pulsars including the first ever discovered millisecond pulsar (MSP). We are conducting an image-based pulsar survey,…

高能天体物理现象 · 物理学 2026-04-01 Yogesh Maan , Apurba Bera , Dharam Vir Lal , Yash Bhusare , Preeti Kharb , Banshi Lal , Pikky Atri