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Related papers: PSR J0737-3039: Interacting Pulsars in X-Rays

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We report the discovery of pulsed {\gamma}-ray emission and X-ray emission from the black widow millisecond pulsar PSR J2051-0827 by using the data from the Large Area Telescope (LAT) on board the Fermi Gamma-ray Space Telescope and the…

High Energy Astrophysical Phenomena · Physics 2015-06-03 J. H. K. Wu , A. K. H. Kong , R. H. H. Huang , J. Takata , P. H. T. Tam , E. M. H. Wu , K. S. Cheng

We report the detection of the millisecond pulsar B1257+12 with the Chandra X-ray Observatory. In a 20 ks exposure we detected 25 photons from the pulsar, with energies between 0.4 and 2.0 keV, corresponding to the flux F_X=(4.4+/-…

Astrophysics · Physics 2009-06-23 G. G. Pavlov , O. Kargaltsev , G. P. Garmire , A. Wolszczan

We report the discovery of pulsed X-ray emission from the compact object CXOU J112439.1-591620 within the supernova remnant (SNR) G292.0+1.8 using the High Resolution Camera on the Chandra X-ray Observatory. The X-ray period (P=0.13530915…

PSR B0943+10 is a mode-switching radio pulsar characterized by two emission modes with different radio and X-ray properties. Previous studies, based on simple combinations of blackbody and power law models, showed that its X-ray flux can be…

High Energy Astrophysical Phenomena · Physics 2019-02-13 Michela Rigoselli , Sandro Mereghetti , Roberto Turolla , Roberto Taverna , Valery Suleimanov , Alexander Y. Potekhin

The spectral energy distribution from the X-ray to the very high energy regime ($>100$ GeV) has been investigated for the $\gamma$-ray binary system PSR B1259-63/SS2883 as a function of orbital phase within the framework of a simple model…

High Energy Astrophysical Phenomena · Physics 2009-08-11 Jumpei Takata , Ronald E. Taam

We report a 72 ks XMM-Newton observation of the Be/X-ray pulsar (BeXRP) RX J0812.4-3114 in quiescence ($L_X \approx 1.6 \times 10^{33}~\mathrm{erg~s^{-1}}$). Intriguingly, we find a two component spectrum, with a hard power-law ($\Gamma…

High Energy Astrophysical Phenomena · Physics 2019-07-24 Yue Zhao , Craig O. Heinke , Sergey S. Tsygankov , Wynn C. G. Ho , Alexander Y. Potekhin , Aarran W. Shaw

We detected X-ray emission from PSR B1800-21 and its synchrotron nebula with the Chandra X-ray Observatory. The pulsar's observed flux is (1.4+/-0.2) 10^{-14} ergs cm^{-2} s^{-1} in the 1-6 keV band. The spectrum can be described by a…

Astrophysics · Physics 2011-02-11 O. Kargaltsev , G. G. Pavlov , G. P. Garmire

The low-mass X-ray binary (LMXB) system FIRST J102347.6+003841 hosts a newly born millisecond pulsar (MSP) PSR J1023+0038 that was revealed as the first and only known rotation-powered MSP in a quiescent LMXB. While the system is shown to…

X-ray emission is generally believed to be one of the major heating sources for the optical modulation in redback pulsar binaries as we have seen similar phenomena in many low mass X-ray binaries (LMXBs). While, e.g., MeV/GeV gamma-rays…

High Energy Astrophysical Phenomena · Physics 2025-10-10 Ka-Yui Au , Kwan-Lok Li , Albert K. H. Kong , Jumpei Takata , Chung-Yue Hui , Lupin C. C. Lin

We present multiwavelength studies of the 106.6 ms gamma-ray pulsar PSR J1907+06 near the TeV source MGRO J1908+06. Timing observations with Fermi result in a precise position determination for the pulsar of R.A. = 19h07m547(2), decl. =…

High Energy Astrophysical Phenomena · Physics 2015-05-14 Fermi LAT Collaboration , the Fermi Pulsar Timing Consortium , : , A. A. Abdo

The origin and radiation mechanisms of high energy emissions from pulsars have remained mysterious since their discovery. Here we report, based on a sample of 68 pulsars, observational connection of non-thermal X-ray emissions from pulsars…

High Energy Astrophysical Phenomena · Physics 2023-02-15 Hsiang-Kuang Chang , Jr-Yue Hsiang , Che-Yen Chu , Yun-Hsin Chung , Tze-Hsiang Su , Tzu-Hsuan Lin , Chien-You Huang

We analyze new XMM-Newton and archival Chandra observations of the middle-aged $\gamma$-ray radio-quiet pulsar J1957+5033. We detect, for the first time, X-ray pulsations with the pulsar spin period of the point-like source coinciding by…

High Energy Astrophysical Phenomena · Physics 2022-06-09 D. A. Zyuzin , A. V. Karpova , Y. A. Shibanov , A. Y. Potekhin , V. F. Suleimanov

We report on Bayesian parameter estimation of the mass and equatorial radius of the millisecond pulsar PSR J0030$+$0451, conditional on pulse-profile modeling of Neutron Star Interior Composition Explorer (NICER) X-ray spectral-timing event…

PSR J0537-6910 is a young, energetic, rotation-powered X-ray pulsar with a spin period of 16 ms located in the Large Magellanic Cloud. We have searched for previously undetected radio pulsations (both giant and standard) from this pulsar in…

Astrophysics · Physics 2008-11-26 F. Crawford , M. McLaughlin , S. Johnston , R. Romani , E. Sorrelgreen

The binary millisecond radio pulsar PSR J1023+0038 has been recently the subject of multiwavelength monitoring campaigns which revealed that an accretion disc has formed around the neutron star (since 2013 June). We present here the results…

We present here timing and spectral analyses of SGR J1830$-$0645 based on an AstroSat observation carried out on 2020 October 16, about a week after the onset of its first detected X-ray outburst. Using data taken with the Soft X-ray…

High Energy Astrophysical Phenomena · Physics 2023-10-17 Rahul Sharma , Chetana Jain , Biswajit Paul , T. R. Seshadri

We report on Chandra ACIS and XMM-Newton MOS/PN imaging observations of two pulsar wind nebulae (K3/PSR J1420-6048 and G313.3+0.1=`the rabbit') associated with the Galactic unidentified gamma-ray source GeV J1417-6100. With the excellent…

Astrophysics · Physics 2009-11-10 C. -Y. Ng , Mallory S. E. Roberts , Roger W. Romani

We present the results of detailed X-ray analysis of two black-widow pulsars (BWPs), J1446-4701 and J1311-3430. PSR J1446-4701 is a BWP with orbital parameters near the median values of the sample of known BWPs. Its X-ray emission detected…

High Energy Astrophysical Phenomena · Physics 2015-10-26 Prakash Arumugasamy , George G. Pavlov , Gordon P. Garmire

New simultaneous X-ray and radio observations of the archetypal mode-switching pulsar PSR B0943+10 have been carried out with XMM-Newton and the LOFAR, LWA and Arecibo radio telescopes in November 2014. They allowed us to better constrain…

NICER observed several rotation-powered millisecond pulsars to search for or confirm the presence of X-ray pulsations. When broad and sine-like, these pulsations may indicate thermal emission from hot polar caps at the magnetic poles on the…