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In a multi-orbit (100 ks) $\mathrm{\it XMM-Newton}$ exposure of the original black widow pulsar, PSR J1959+2048, we measure the strong orbital modulation caused by intrabinary shock (IBS) emission. The IBS light curve peak appears…

High Energy Astrophysical Phenomena · Physics 2021-08-25 D. Kandel , Roger W. Romani , Hongjun An

Eclipsing millisecond pulsars in close ($P_b < 1$~day) binary systems provide a different view of pulsar winds and shocks than do isolated pulsars. Since 2009, the numbers of these systems known in the Galactic field has increased…

High Energy Astrophysical Phenomena · Physics 2015-06-18 Mallory S. E. Roberts , Maura A. McLaughlin , Peter Gentile , Ester Aliu , Jason W. T. Hessels , Scott M. Ransom , Paul S. Ray

The low mass companions of evaporating binary pulsars (black widows and their ilk) are strongly heated on the side facing the pulsar. However in high-quality photometric and spectroscopic data the heating pattern does not match that…

High Energy Astrophysical Phenomena · Physics 2016-08-31 Roger W. Romani , Nicolas Sanchez

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

Black widow and redback systems are compact binaries in which a millisecond pulsar heats and may even ablate its low-mass companion by its intense wind of relativistic particles and radiation. In such systems, an intrabinary shock can form…

High Energy Astrophysical Phenomena · Physics 2020-12-02 Christian J. T. van der Merwe , Zorawar Wadiasingh , Christo Venter , Alice K. Harding , Matthew G. Baring

The intrabinary shocks (IBS) of spider pulsars emit non-thermal synchrotron X-rays from accelerated electrons and positrons in the shocked pulsar wind, likely energized by magnetic reconnection. In redback spider pulsars, the IBS typically…

High Energy Astrophysical Phenomena · Physics 2025-04-03 Andrew G. Sullivan , Roger W. Romani

A large number of new "black widow" and "redback" energetic millisecond pulsars with irradiated stellar companions have been discovered through radio and optical searches of unidentified \textit{Fermi} sources. Synchrotron emission, from…

High Energy Astrophysical Phenomena · Physics 2016-02-23 Zorawar Wadiasingh , Alice K. Harding , Christo Venter , Markus Boettcher

The intrabinary shocks (IBS) in spider pulsars emit non-thermal synchrotron X-rays from accelerated electrons and positrons in the shocked pulsar wind, likely energized by magnetic reconnection. The double-peaked X-ray light curves from…

High Energy Astrophysical Phenomena · Physics 2026-01-19 Andrew G. Sullivan , Jack T. Dinsmore , Roger W. Romani

In `spider' pulsars, the X-ray band is dominated by Intrabinary Shock (IBS) synchrotron emission. While the double-peaked X-ray light curves from these shocks have been well characterized in several spider systems (both black widows and…

High Energy Astrophysical Phenomena · Physics 2023-11-08 Andrew G. Sullivan , Roger W. Romani

'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…

High Energy Astrophysical Phenomena · Physics 2026-02-12 Christo Venter , Andreas Kopp , Zorawar Wadiasingh , Alice K Harding , M Baring

A large number of new black widow and redback energetic millisecond pulsars with irradiated stellar companions have been discovered through radio searches of unidentified \emph{Fermi} sources. We construct a 3D emission model of these…

High Energy Astrophysical Phenomena · Physics 2015-12-24 Zorawar Wadiasingh , Alice K. Harding , Christo Venter , Markus Böttcher

Spider pulsars are binary systems composed of a millisecond pulsar and a low-mass companion. Their X-ray emission, varying with orbital phase, originates from synchrotron radiation produced by high-energy electrons accelerated at the…

High Energy Astrophysical Phenomena · Physics 2025-01-16 Jorge Cortés , Lorenzo Sironi

PSR J2215+5135 (J2215) is a `redback' spider pulsar, where the intrabinary shock (IBS) wraps around the pulsar rather than the stellar-mass companion. Spider orbital light curves are modulated, dominated by their binary companion thermal…

High Energy Astrophysical Phenomena · Physics 2024-09-05 Andrew G. Sullivan , Roger W. Romani

We report on high-energy properties of the black widow pulsar PSR J2241$-$5236 in the X-ray and the Fermi-LAT (GeV gamma-ray) bands. In the LAT band, the phase-averaged gamma-ray light curve shows orbital modulation below $\sim$1 GeV with a…

High Energy Astrophysical Phenomena · Physics 2018-11-28 Hongjun An , Roger W. Romani , Matthew Kerr

We investigated a wealth of X-ray and gamma-ray spectral energy distribution (SED) and multi-band light curve (LC) data of the gamma-ray binary HESS J0632+057 using a phenomenological intrabinary shock (IBS) model. Our baseline model…

High Energy Astrophysical Phenomena · Physics 2022-09-07 Jinyoung Kim , Hongjun An , Kaya Mori

Spectrally hard X-ray emission with double-peak light curves (LCs) and orbitally modulated gamma rays have been observed in some millisecond pulsar binaries, phenomena attributed to intrabinary shocks (IBSs). While the existing IBS model by…

High Energy Astrophysical Phenomena · Physics 2024-11-11 Jaegeun Park , Chanho Kim , Hongjun An , Zorawar Wadiasingh

The companions of evaporating binary pulsars (black widows and related systems) show optical emission suggesting strong heating. In a number of cases large observed temperatures and asymmetries are inconsistent with direct radiative heating…

High Energy Astrophysical Phenomena · Physics 2017-08-23 Nicholas Sanchez , Roger W. Romani

Black widows and redbacks are binary systems consisting of a millisecond pulsar in a close binary with a companion having matter driven off of its surface by the pulsar wind. X-rays due to an intra-binary shock have been observed from many…

Redback millisecond pulsars (MSPs) typically show pronounced orbital variability in their X-ray emission due to our changing view of the intrabinary shock (IBS) between the pulsar wind and stellar wind from the companion. Some redbacks…

High Energy Astrophysical Phenomena · Physics 2020-10-14 Pavan R. Hebbar , Craig O. Heinke , D. Kandel , Roger W. Romani , P. C. C. Freire

Multiwavelength followup of unidentified Fermi sources has vastly expanded the number of known galactic-field "black widow" and "redback" millisecond pulsar binaries. Focusing on their rotation-powered state, we interpret the radio to X-ray…

High Energy Astrophysical Phenomena · Physics 2017-04-26 Zorawar Wadiasingh , Alice K. Harding , Christo Venter , Markus Böttcher , Matthew G. Baring
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