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Related papers: Two Possible Optical--X-Ray Anti-Correlations of P…

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We have investigated the X-ray and $\gamma$-ray properties of the redback millisecond pulsar PSR J1723-2837 with XMM-Newton, Chandra and Fermi. We have discovered the X-ray orbital modulation of this binary system with the minimum that…

High Energy Astrophysical Phenomena · Physics 2015-06-17 C. Y. Hui , P. H. T. Tam , J. Takata , A. K. H. Kong , K. S. Cheng , J. H. K. Wu , L. C. C. Lin , E. M. H. Wu

We investigated the multiband emission from the pulsar binaries XSS J12270-4859, PSR J2039-5617, and PSR J2339-0533, which exhibit orbital modulation in the X-ray and gamma-ray bands. We constructed the sources' broadband spectral energy…

High Energy Astrophysical Phenomena · Physics 2024-02-06 Minju Sim , Hongjun An , Zorawar Wadiasingh

We present X-ray observations of the "redback" eclipsing radio millisecond pulsar and candidate radio pulsar/X-ray binary transition object PSR J1723-2837. The X-ray emission from the system is predominantly non-thermal and exhibits…

High Energy Astrophysical Phenomena · Physics 2015-06-17 Slavko Bogdanov , Paolo Esposito , Fronefield Crawford , Andrea Possenti , Maura A. McLaughlin , Paulo Freire

We have investigated the intrabinary shock emission from the redback millisecond pulsar PSR J2129-0429 with XMM-Newton and Fermi. Orbital modulation in X-ray and UV can be clearly seen. Its X-ray modulation has a double-peak structure with…

High Energy Astrophysical Phenomena · Physics 2015-06-23 C. Y. Hui , C. P. Hu , S. M. Park , J. Takata , K. L. Li , P. H. T. Tam , L. C. C. Lin , A. K. H. Kong , K. S. Cheng , Chunglee Kim

We present the first X-ray observation of the energetic millisecond pulsar binary PSR J1431-4715, performed with XMM-Newton and complemented with fast optical multi-band photometry acquired with the ULTRACAM instrument at ESO-NTT. It is…

High Energy Astrophysical Phenomena · Physics 2024-09-04 D. de Martino , A. Phosrisom , V. S. Dhillon , D. F. Torres , F. Coti Zelati , R. P. Breton , T. R. Marsh , A. Miraval Zanon , N. Rea , A. Papitto

We report on orbital modulation of the 100-600 MeV gamma-ray emission of the $P_{\rm B}=4.6$ hr millisecond pulsar binary PSR J2339$-$0533 using 11 yr of Fermi Large Area Telescope data. The modulation has high significance (chance…

High Energy Astrophysical Phenomena · Physics 2020-07-08 Hongjun An , Roger W. Romani , Matthew Kerr

We report on the XMM-Newton observations of the 143 ms pulsar PSR J0538+2817. We present evidence for the first detections of pulsed X-rays from the source at a frequency which is consistent with the predicted radio frequency. The pulse…

We are monitoring established and putative redback millisecond pulsars (MSPs) in time-series photometry, repeatedly covering their 5-6 hr orbital light curves in $r^{\prime}$ or $R$. On timescales of months, PSR J1048+2339 and XMMU…

High Energy Astrophysical Phenomena · Physics 2018-10-24 Patricia B. Cho , Jules P. Halpern , Slavko Bogdanov

The spectra of several X-ray binary pulsars display a clear soft excess, which in most cases can be described with a blackbody model, above the main power-law component. While in the high-luminosity sources it is usually characterized by…

High Energy Astrophysical Phenomena · Physics 2015-05-13 N. La Palombara , L. Sidoli , P. Esposito , A. Tiengo , S. Mereghetti

Optical/near-infrared (optical/NIR; OIR) light from low-mass neutron star X-ray binaries (NSXBs) in outburst is traditionally thought to be thermal emission from the accretion disc. Here we present a comprehensive collection of…

Astrophysics · Physics 2009-06-23 D. M. Russell , R. P. Fender , P. G. Jonker

We have completed part of a program to study the X-ray emission properties of old rotation-powered pulsars with XMM-Newton in order to probe and identify the origin of their X-radiation. The X-ray emission from these old pulsars is largely…

Transitional pulsars provide us with a unique laboratory to study the physics of accretion onto a magnetic neutron star. PSR J1023+0038 (J1023) is the best studied of this class. We investigate the X-ray spectral properties of J1023 in the…

High Energy Astrophysical Phenomena · Physics 2019-09-25 S. Campana , A. Miraval Zanon , F. Coti Zelati , D. F. Torres , M. C. Baglio , A. Papitto

The observed radio-optical-X-ray spectral energy distributions (SEDs) of 22 hot spots and 45 knots in the jets of 35 active galactic nuclei are complied from literature and modeled with single-zone lepton models. It is found that the…

High Energy Astrophysical Phenomena · Physics 2014-11-20 Jin Zhang , J. M. Bai , Liang Chen , Enwei Liang

The PSR J1023+0038 binary system hosts a neutron star and a low-mass, main-sequence-like star. It switches on year timescales between states as an eclipsing radio millisecond pulsar and a low-mass X-ray binary. We present a multi-wavelength…

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…

High Energy Astrophysical Phenomena · Physics 2022-08-31 Jules P. Halpern , Karen I. Perez , Slavko Bogdanov

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…

The study of high-magnetic-field pulsars is important for examining the relationships between radio pulsars, magnetars, and X-ray-isolated neutron stars (XINSs). Here we report on X-ray observations of three such high-magnetic-field radio…

High Energy Astrophysical Phenomena · Physics 2013-09-18 S. A. Olausen , W. W. Zhu , J. K. Vogel , V. M. Kaspi , A. G. Lyne , C. M. Espinoza , B. W. Stappers , R. N. Manchester , M. A. McLaughlin

We present the first results from a joint XMM-Newton and NuSTAR observation of the gamma-ray emitting millisecond pulsar compact binary PSR J2129-0429. X-ray emission up to about 40 keV is detected and the joint spectrum can be modeled with…

High Energy Astrophysical Phenomena · Physics 2018-07-11 A. K. H. Kong , J. Takata , C. Y. Hui , J. Zhao , K. L. Li , P. H. T. Tam

We present results from a deep search for radio emission from the X-ray pulsar systems GX 1+4, GS 0834-430 and 4U 0115+63 which have variously been suggested to possess radio jets and to be good candidates for propellor ejection mechanisms.…

We obtained new optical observations of the X-ray source XMMU J083850.38-282756.8, the previously proposed counterpart of the gamma-ray source 3FGL J0838.8-2829. Time-series photometry in the $r'$ band reveals periodic modulation of…

High Energy Astrophysical Phenomena · Physics 2017-08-09 J. P. Halpern , J. Strader , M. Li
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