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Related papers: X-Ray Studies of Redbacks

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Millisecond pulsars (MSPs) are mainly characterised by their spin periods, B-fields and masses - quantities which are largely affected by previous interactions with a companion star in a binary system. In this paper, we investigate the…

Solar and Stellar Astrophysics · Physics 2012-08-30 Thomas M. Tauris , Norbert Langer , Michael Kramer

We report the discovery of peculiar X-ray spectral variability in the binary radio millisecond pulsar PSR J0024--7204W in the globular cluster 47 Tucanae. The observed emission consists of a dominant non-thermal component, which is eclipsed…

Astrophysics · Physics 2009-11-11 Slavko Bogdanov , Jonathan E. Grindlay , Maureen van den Berg

A number of low-mass millisecond pulsar (MSP) binaries in their rotation-powered state exhibit double-peaked X-ray orbital modulation centered at inferior pulsar conjunction. This state, which has been known to persist for years, has…

High Energy Astrophysical Phenomena · Physics 2018-12-26 Zorawar Wadiasingh , Christo Venter , Alice K. Harding , Markus Böttcher , Patrick Kilian

PSR\,J1723$-$2837 is a "redback" millisecond pulsar (MSP) with a low-mass companion in a 14.8\,h orbit. The system's properties closely resemble those of "transitional" MSPs that alternate between spin-down and accretion-powered states. In…

Solar and Stellar Astrophysics · Physics 2016-12-08 André van Staden , John Antoniadis

We describe the first X-ray observations of binary millisecond pulsars PSRs J0023+0923, J1810+1744, J2215+5135, and J2256-1024. All four are Fermi gamma-ray sources and three are 'black-widow' pulsars, with companions of mass < 0.1 solar…

Solar and Stellar Astrophysics · Physics 2015-06-11 Peter Gentile , Maura McLaughlin , Mallory Roberts , Fernando Camilo , Jason Hessels , Matthew Kerr , Scott Ransom , Paul Ray , Ingrid Stairs

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

We present optical observations of the redback millisecond pulsar PSR J1048+2339, which is a 4.66 ms radio pulsar in a compact binary with an orbital period of six hours. We obtained high-quality light curves of PSR J1048+2339 with the…

High Energy Astrophysical Phenomena · Physics 2019-01-16 Yee Xuan Yap , K. L. Li , A. K. H. Kong , J. Takata , J. Lee , C. Y. Hui

We report on XMM-Newton observations of the "Black Widow pulsar", PSR B1957+20. The pulsar's X-ray emission is non-thermal and best modeled with a single powerlaw spectrum of photon index 2.03(+0.51/-0.36). No coherent X-ray pulsations at…

Astrophysics · Physics 2007-05-23 Hsiu-Hui Huang , Werner Becker

We present high time resolution SDSS-$g'$ and SDSS-$z'$ light curves of the primary eclipse in SDSS J141126.20+200911.1, together with time-resolved X-Shooter spectroscopy and near-infrared $JHK_{s}$ photometry. Our observations confirm the…

We have observed the persistent but optically unidentified X-ray source X1908+075 with the PCA and HEXTE instruments on RXTE. The binary nature of this source was established by Wen, Remillard, & Bradt (2000) who found a 4.4-day orbital…

Astrophysics · Physics 2009-11-10 A. M. Levine , S. Rappaport , R. Remillard , A. Savcheva

In this review I discuss the characteristics and the formation of all classes of millisecond pulsars (MSPs). The main focus is on the stellar astrophysics of X-ray binaries leading to the production of fully recycled MSPs with white dwarf…

High Energy Astrophysical Phenomena · Physics 2015-03-19 Thomas M. Tauris

The discovery of millisecond pulsars switching between states powered either by the rotation of their magnetic field or by the accretion of matter, has recently proved the tight link shared by millisecond radio pulsars and neutron stars in…

High Energy Astrophysical Phenomena · Physics 2015-04-28 A. Papitto , D. F. Torres

XMM-Newton and Chandra observations of the transient 7.8 s pulsar XTE J1829-098 are used to characterize its pulse shape and spectrum, and to facilitate a search for an optical or infrared counterpart. In outburst, the absorbed, hard X-ray…

Astrophysics · Physics 2009-11-13 J. P. Halpern , E. V. Gotthelf

We report NuSTAR observations of the millisecond pulsar - low mass X-ray binary (LMXB) transition system PSR J1023+0038 from June and October 2013, before and after the formation of an accretion disk around the neutron star. Between June…

We report on XMM-Newton observations of the Black Widow pulsar, PSR B1957+20. The pulsar's X-ray emission is non-thermal and best modeled with a single powerlaw spectrum of photon index 2.03^{+0.51}_{-0.36}. No coherent X-ray pulsations at…

Astrophysics · Physics 2015-06-24 H. H. Huang , W. Becker

We report on the first NuSTAR observation of the transitional millisecond pulsar binary XSS J12270-4859 during its current rotation-powered state, complemented with a 2.5yr-long radio monitoring at Parkes telescope and archival XMM-Newton…

High Energy Astrophysical Phenomena · Physics 2020-01-24 D. de Martino , A. Papitto , M. Burgay , A. Possenti , F. Coti Zelati , N. Rea , D. F. Torres , T. M. Belloni

We have performed detailed numerical calculations of the non-conservative evolution of close binary systems with low-mass (1.0-2.0 M_sun) donor stars and a 1.3 M_sun accreting neutron star. Rather than using analytical expressions for…

Astrophysics · Physics 2007-05-23 T. M. Tauris , G. J. Savonije

We present ULTRACAM multiband optical photometry of two transitional millisecond pulsars, PSR J1023+0038 and PSR J1227$-$4853, taken while both were in their radio pulsar states. The light curves show significant asymmetry about the flux…

The population of millisecond pulsars (MSPs) has been expanded considerably in the last decade. Not only is their number increasing, but also various classes of them have been revealed. Among different classes of MSPs, the behaviour of…

High Energy Astrophysical Phenomena · Physics 2019-12-17 C. Y. Hui , K. L. Li

We present a new analysis of the light curve for the secondary star in the eclipsing binary millisecond pulsar system PSR B1957+20. Combining previous data and new data points at minimum from the Hubble Space Telescope, we have 100%…